Welding Stainless Steel, Aluminum and Copper Alloys

Welding Stainless Steel, Aluminum & Copper — Metallurgy Guide | WeldFabWorld

Welding Stainless Steel, Aluminum and Copper Alloys: Metallurgical Considerations

Welding stainless steel, aluminum, and copper alloys each presents a distinct set of metallurgical challenges that do not exist in conventional carbon steel fabrication. While carbon steel dominates welding education, a large and growing proportion of industrial welded fabrication involves these three material families — in chemical process plant, offshore structures, food and pharmaceutical equipment, heat exchangers, and power generation systems. The inspector or engineer who understands only carbon steel metallurgy is under-equipped for a significant portion of real-world fabrication work.

Unlike carbon steels, where the primary concerns centre on hardenability, hydrogen cracking, and PWHT, these three material families introduce entirely different phenomena: sensitisation and intergranular corrosion in austenitic stainless steel; a tenacious refractory oxide film that must be physically removed before welding aluminum; and the destruction of cold-worked strength properties in copper alloys by the welding thermal cycle. Each material demands specific process selection, filler metal matching, and procedure controls that cannot be extrapolated from carbon steel practice.

This guide covers the metallurgical mechanisms underlying each challenge — sensitisation, carbide precipitation, delta ferrite control, hot cracking, oxide film removal, alloy series identification, and thermal conductivity effects — and the practical measures used to manage them. Filler metal selection, code references, and inspector monitoring guidance are included throughout. For background on the iron-carbon system and solid-state transformations, refer to the martensite, bainite and pearlite guide in the WeldFabWorld metallurgy series.

≥12%
Minimum Cr for stainless steel passive film formation
427–871 °C
Sensitisation temperature range for austenitic stainless
4–10 FN
Target delta ferrite range to prevent hot cracking
2049 °C
Melting point of Al₂O₃ oxide film on aluminum
Article Scope: This article covers austenitic, ferritic, martensitic, and duplex stainless steels; wrought aluminum alloys (1xxx–7xxx series); and copper and copper alloy groups including copper-nickel, brass, and bronze. Nickel alloys and titanium are treated separately in dedicated WeldFabWorld articles.

Part 1: Stainless Steels

Definition and the Passive Film

Stainless steels are defined as iron-based alloys containing a minimum of 10.5–12% chromium by mass. The chromium reacts spontaneously with atmospheric oxygen to form a thin, adherent, self-repairing chromium oxide (Cr₂O₃) layer — the “passive film” — typically only 2–5 nanometres thick. This invisible film is what provides the corrosion resistance for which stainless steels are valued. If the chromium content in any localised region falls below approximately 12%, the passive film cannot sustain itself and the material corrodes as ordinary iron would. This mechanism is central to understanding the most important welding problem in austenitic stainless steel: sensitisation.

Despite the “stainless” descriptor, these alloys can and do corrode under sufficiently aggressive conditions. The Pitting Resistance Equivalent Number (PREN) — PREN = %Cr + 3.3 × %Mo + 16 × %N — is a widely used index of resistance to localised (pitting) corrosion. When welding stainless steel, it is important to verify that the weld deposit PREN is not substantially lower than that of the base material, since dilution and element burn-off can reduce local corrosion resistance at the weld.

Classification of Stainless Steels

The five main classes of stainless steel are differentiated by their room-temperature microstructure, which in turn is controlled by the balance of austenite-forming (Ni, N, Mn, C) and ferrite-forming (Cr, Mo, Si, Nb, Ti) elements.

Class Typical Grades Microstructure P-No. (ASME IX) Weldability
Austenitic 304, 304L, 316, 316L, 321, 347 FCC austenite P-No. 8 Excellent
Ferritic 409, 430, 444 BCC ferrite P-No. 7 Good — proper fillers required
Martensitic 410, 416, 420, 431 BCT martensite P-No. 6 Requires preheat & PWHT
Duplex 2205 (UNS S31803), 2507, LDX2101 ~50% austenite / ~50% ferrite P-No. 10H Weldable; ferrite control critical
Precipitation Hardening 17-4 PH (630), 15-5 PH Martensitic or semi-austenitic P-No. 6 / 8 PWHT mandatory to restore properties
Simplified Schaeffler Constitution Diagram — Stainless Steel Weld Microstructures Chromium Equivalent (Crₛq = %Cr + %Mo + 1.5×%Si + 0.5×%Nb) → Nickel Equivalent (Niₛq = %Ni + 30×%C + 0.5×%Mn) → 10 15 20 25 30 35 0 5 10 15 20 Martensite 410, 420 M+A Austenite 304, 316, 321, 347 Duplex A+F 2205, 2507 Ferrite 409, 430 Target: 4–10 FN Delta Ferrite 304 (ER308L) 316 (ER316L) 2205
Figure 1 — Simplified Schaeffler constitution diagram for stainless steel weld metal. The target 4–10 FN delta ferrite band falls within the duplex/austenite boundary region, preventing solidification hot cracking. Austenitic grades 304 and 316 with matching fillers should fall within this band.

Austenitic Stainless Steels: Sensitisation and Carbide Precipitation

Austenitic stainless steels (the 200 and 300 series, including the widely used 304 and 316) are generally considered the most weldable of the stainless families. They are not hardenable by quenching, they do not transform to martensite during welding (in properly balanced compositions), and they require neither preheat nor PWHT for structural integrity purposes. However, they are susceptible to a specific and critically important metallurgical degradation mechanism called sensitisation — also referred to as carbide precipitation or weld decay when the resulting corrosion occurs in service.

The Mechanism of Sensitisation

During welding, the HAZ is heated through a range of temperatures. In the specific range of approximately 427–871 °C (800–1600 °F), both chromium and carbon dissolved in the austenite matrix have sufficient atomic mobility to diffuse to grain boundaries and combine. The compound formed is primarily chromium carbide — Cr₃₂C₆ — which precipitates as a discontinuous network along austenite grain boundaries. The most active temperature for this reaction is approximately 677 °C (1250 °F).

As carbide precipitates at the grain boundary, the chromium required to form it is drawn from the immediately adjacent matrix. Because solid-state diffusion is slow at these temperatures, the chromium-depleted zone cannot replenish itself from the bulk. The result is a narrow band on either side of each grain boundary where chromium content may drop below 12% — below the threshold required for passive film formation. This phenomenon is called chromium depletion.

Service Consequence: In corrosive environments, the chromium-depleted grain boundary zones corrode preferentially while the grain interiors (unaffected by sensitisation) remain passive. The result is intergranular corrosion (IGC) or intergranular attack (IGA) — a form of corrosion that follows grain boundaries and can cause the material to crumble or disintegrate with little visible surface evidence. Testing per ASTM A262 is used to evaluate susceptibility to IGC.

Three Methods to Prevent Sensitisation

  1. Extra Low Carbon (ELC / “L” grades) — 304L, 316L: Limiting carbon to a maximum of 0.03% (versus 0.08% for standard grades) dramatically reduces the amount of carbon available to combine with chromium. Less carbon means less Cr₃₂C₆ can form, and the chromium depletion is insufficient to cause loss of passivity. The trade-off is a modest reduction in elevated-temperature mechanical properties. For ambient and moderate-temperature service this is usually acceptable.
  2. Stabilised Grades — 321 (Ti-stabilised) and 347 (Nb-stabilised): Titanium and niobium have a stronger thermodynamic affinity for carbon than chromium does. In these grades, the carbon combines preferentially with Ti or Nb to form stable, dispersed carbide particles (TiC, NbC), consuming the carbon before it can form Cr₃₂C₆. The chromium remains in solid solution and the passive film is maintained throughout the weld thermal cycle. Stabilised grades are preferred for applications operating continuously at 425–870 °C (such as boiler superheaters and heat exchangers).
  3. Post-Weld Solution Annealing: Heating to 1050–1100 °C and holding sufficiently long to re-dissolve all chromium carbides back into solid solution, followed by rapid water quench to suppress re-precipitation. This fully restores corrosion resistance but often causes severe distortion of complex weldments and is impractical for large structures or assembled equipment. It is most commonly used for small, simple components or critical pressure-retaining parts.
Inspector Tip: When a procedure specifies 316L filler for a 316 base metal weld, confirm the actual test certificate carbon content — not just the grade designation. A heat of “316L” can have carbon as high as 0.030%, but some heats are as low as 0.015%. For highly aggressive service (concentrated acids, seawater), the actual carbon content matters. See the stainless steel weld decay guide for IGC testing standards including ASTM A262 Practice E.

Hot Short Cracking (Solidification Cracking) in Austenitic Stainless Steel

The second major welding problem for austenitic stainless steels is solidification cracking, commonly called hot short cracking or hot cracking. This occurs during or immediately after solidification of the weld pool. The mechanism involves low-melting-point impurity films — enriched in sulphur, phosphorus, and silicon — that persist as liquid films along solidifying grain boundaries when the weld metal bulk has already solidified. As the weld metal contracts on cooling, these liquid films cannot accommodate the thermal strain, and they tear open as cracks along grain boundaries.

Delta Ferrite as the Solution

The proven solution is to control weld metal composition such that a small fraction of delta ferrite (δ-ferrite) — a BCC iron phase — is present in the as-solidified weld bead. Delta ferrite provides several benefits:

  • Delta ferrite has significantly higher solubility for sulphur and phosphorus than austenite, absorbing these impurities and preventing them from forming liquid films at grain boundaries
  • The delta ferrite-austenite grain boundaries created during solidification interrupt the continuous grain boundary network through which hot cracks would otherwise propagate
  • The solidification mode shifts from a purely austenitic path (crack-susceptible) to a ferritic-austenitic path (crack-resistant) when delta ferrite is present
Target Ferrite Number: A delta ferrite content of 4 to 10 FN (Ferrite Number) in the as-deposited weld metal effectively prevents hot cracking. The Ferrite Number can be predicted from weld metal composition using the WRC-1992 constitution diagram (superior to the older Schaeffler diagram for modern stainless steels) or measured directly on the completed weld using a calibrated magnetic gage (ferritescope or magne-gage), since delta ferrite is ferromagnetic while austenite is non-magnetic. ASME Section IX QW-442 and AWS A4.2 govern Ferrite Number measurement procedures.
Base Metal Grade Standard Filler Alternate Filler Target FN Key Concern
304 / 304L ER308 / ER308L ER308LSi 4–10 FN Sensitisation (use L-grade)
316 / 316L ER316 / ER316L ER316LSi 4–10 FN Pitting resistance (Mo content)
321 (Ti-stabilised) ER347 (Nb-stabilised) ER321 4–10 FN Ti lost to arc — use 347 filler
347 (Nb-stabilised) ER347 ER308L 4–10 FN High-temperature service stability
310 (High-Si, high-Cr) ER310 ERNiCr-3 0 FN (fully austenitic) Hot cracking risk — control S, P
2205 Duplex ER2209 ERNiCrMo-3 30–55 FN (duplex) See duplex stainless guide
Note on Fully Austenitic Grades: High-alloy fully austenitic grades (310, 330, AL-6XN, 904L, and most nickel alloys) cannot tolerate delta ferrite — it would precipitate sigma phase in elevated temperature service. For these grades, hot cracking risk is managed by strict control of base metal and filler metal sulphur and phosphorus content (typically S < 0.010%), high heat input avoidance, and use of GTAW processes that minimise dilution. Refer to the delta ferrite importance guide for full details.

Ferritic Stainless Steels

Ferritic stainless steels (grades 409, 430, 444) maintain a BCC ferritic structure at all temperatures — they cannot be hardened by quenching. Their weldability is generally good, but several specific issues require attention:

  • Grain coarsening: Ferritic stainless steels have no austenite-to-ferrite transformation during cooling to refine the grain structure (unlike carbon steels). The weld HAZ grains grow rapidly and remain coarse, significantly reducing impact toughness. Keeping heat input low is essential.
  • 475 °C Embrittlement: Extended exposure at 370–540 °C causes precipitation of a chromium-rich alpha-prime phase that dramatically reduces toughness and ductility. Slow cooling through this range during PWHT must be avoided.
  • Filler metal selection: Using an austenitic filler (e.g. ER309L) rather than a matching ferritic filler can improve weld metal toughness by depositing a ductile austenitic or duplex weld metal, though this introduces a dissimilar interface that may behave differently in service.

Martensitic Stainless Steels

Martensitic grades (410, 416, 420, 431) are the most challenging of the stainless steels to weld. They have significant hardenability and transform from austenite to brittle martensite in the HAZ during the welding thermal cycle, in direct analogy with hardenable carbon steels. Grade 410, for example, can develop HAZ hardness exceeding 400 HV — well into the range susceptible to hydrogen-induced cold cracking.

Typical Procedure Requirements for Martensitic Stainless (Grade 410):
Preheat: 150–260 °C (higher for sections >25 mm or carbon >0.10%).
Maximum interpass temperature: 315 °C.
Process: GTAW or low-hydrogen SMAW (E410 or E309/309L filler if toughness is primary).
PWHT: Temper at 650–760 °C for 1 hour per 25 mm minimum, then slow cool. Required to temper HAZ martensite and restore toughness. Do not PWHT in the range 370–565 °C (temper embrittlement risk).
Code reference: ASME Section IX P-No. 6; ASME B31.3 para 331.2.

Part 2: Aluminum and Its Alloys

The Aluminum Oxide Film Challenge

Aluminum is one of the most reactive structural metals in air. When bare aluminum is exposed, a coherent aluminum oxide film (Al₂O₃) forms on the surface within seconds. This oxide film is an exceptional engineering advantage in service — it provides outstanding corrosion resistance even in marine environments — but it creates a severe problem for welding:

2049 °C
Melting point of Al₂O₃ — nearly 3x the base metal melting point
660 °C
Melting point of pure aluminum base metal
<1 sec
Time for oxide film to reform on freshly cleaned aluminum in air

If not removed before and during welding, the oxide film will prevent fusion between the filler metal and base metal, create oxide inclusions in the weld pool, and produce a “cold lap” defect where the weld metal sits on top of an unfused oxide layer rather than truly fusing into the joint. Mechanical pre-cleaning (stainless steel wire brushing, solvent degreasing) is essential before welding, but mechanical cleaning cannot maintain a clean surface during the welding arc — oxide reforms too quickly.

AC GTAW and the Cathodic Cleaning Action

The solution used in GTAW (TIG welding) of aluminum is alternating current (AC). The AC cycle alternates between two half-cycles that serve complementary purposes:

  • Electrode-positive (EP) half-cycle: When current flows from workpiece to electrode, electrons bombard the oxide film surface, breaking it up and dispersing it — the “cathodic cleaning action.” This removes the oxide in real time from ahead of the advancing weld pool.
  • Electrode-negative (EN) half-cycle: When current flows from electrode to workpiece, the arc energy is concentrated at the workpiece, generating the heat needed to melt the base metal and filler. This half-cycle provides the primary fusion energy.

The result is a distinctive “cleaning band” visible either side of the weld bead — a bright, matte zone where the oxide has been removed by cathodic bombardment. Shielding with pure argon prevents re-oxidation within the weld zone during welding. Helium or argon-helium mixtures are sometimes used for deeper penetration on thicker sections.

Process Note: DC electrode-negative (DCEN), the standard polarity for GTAW of steel, provides no cathodic cleaning action and is therefore unsuitable for aluminum welding in most applications. GMAW (MIG welding) of aluminum does use DCEP (DC electrode positive), which provides continuous cathodic cleaning of the base metal surface ahead of the arc; however, the cleaning mechanism in GMAW is less complete than AC GTAW. High-frequency DC GTAW (HFDC or DC+ with square wave) is used in some automated applications for thin gauge aluminum.

The Aluminum Alloy Series and Weldability

Aluminum alloys are classified by a four-digit designation system. The first digit identifies the principal alloying element(s), and the alloy’s weldability and appropriate filler metal selection depend strongly on which series it belongs to.

Series Principal Alloy Strengthening Weldability Typical Filler Example Grades
1xxx Pure Al (≥99%) Work hardening Excellent ER1100, ER1188 1100, 1350
2xxx Copper (Cu) Precipitation hardening Poor — crack-susceptible ER2319 (limited) 2024, 2014, 2219
3xxx Manganese (Mn) Solid solution / work hardening Good ER4043, ER5356 3003, 3004
4xxx Silicon (Si) Solid solution Excellent ER4043, ER4047 4043, 4047 (filler alloys)
5xxx Magnesium (Mg) Solid solution / work hardening Very Good ER5356, ER5183 5052, 5083, 5086
6xxx Mg + Si Precipitation hardening Good with proper filler ER4043, ER5356 6061, 6063, 6082
7xxx Zinc (Zn) Precipitation hardening Limited — specialist procedures ER5356 (limited) 7005, 7075 (generally avoid welding)

Filler Metal Selection for Aluminum — Key Principles

Filler metal selection for aluminum welding is governed by ANSI/AWS A5.10 / ASME SFA-5.10 (Specification for Bare Aluminum and Aluminum Alloy Welding Electrodes and Rods). The primary selection criteria are:

  • Hot crack resistance: The filler must produce a weld deposit that is not susceptible to solidification cracking. Silicon-bearing fillers (4xxx, particularly ER4043 and ER4047) have excellent hot crack resistance. Magnesium-bearing fillers (5xxx, particularly ER5356 and ER5183) also perform well for most 5xxx and 6xxx base metals.
  • Corrosion resistance matching: ER5356 (and higher-Mg fillers) provides better corrosion resistance in marine and chemical environments than ER4043. ER4043 weld deposits are softer and more ductile.
  • Anodising compatibility: If the welded assembly will be anodised, ER4043 deposits may show a different colour than the base metal after anodising (darker/grey), while ER5356 or ER5183 deposits produce a better colour match for 5xxx and 6xxx base metals.
  • Service temperature: ER5356 (containing Mg >3%) should not be used for sustained service above 65 °C due to the risk of sensitisation to stress corrosion in the weld metal. ER4043 or ER5183 is preferred for higher-temperature or marine applications of 5xxx alloys.
6061-T6 and Strength Loss: Grade 6061-T6 is perhaps the most commonly welded heat-treatable aluminum alloy in structural fabrication. The T6 temper (solution annealed and artificially aged) gives yield strength of approximately 275 MPa. After welding, the HAZ is over-aged (softened) to the T4 or annealed condition — yield strength drops to approximately 110–165 MPa in the HAZ. Welded joint design for 6061-T6 must use the post-weld (as-welded or T4-equivalent) strength, not the T6 parent material strength, unless the entire structure is solution-annealed and re-aged after welding. See the GTAW process guide for GTAW setup parameters for aluminum.
HAZ Degradation Mechanisms: Stainless Steel vs. Aluminum Alloys Austenitic SS — Sensitisation 6061-T6 Aluminum — Strength Loss Sensitisation Zone (427–871 °C) Base Sens. ICHAZ Weld ICHAZ Sens. Base Cr depleted zone (chromium <12%) at grain boundaries → passive film breakdown → IGA Prevention: 304L/316L, 321/347, or solution anneal Distance from weld centreline → Yield Strength (MPa) → 275 200 140 0 Base: 275 MPa (T6) HAZ min: ~110–140 MPa HAZ Base metal (T6 condition) Actual yield strength profile Weld deposit (ER4043)
Figure 2 — Left: Sensitisation zones in austenitic stainless steel HAZ where chromium depletion below 12% causes intergranular corrosion susceptibility. Right: Yield strength profile across a 6061-T6 aluminum weld — the HAZ is over-aged to approximately 40–50% of the parent T6 strength. Design must account for the weakest HAZ zone.

Part 3: Copper and Its Alloys

Alloy Families and Strengthening Mechanisms

Copper is one of the oldest engineering metals and is used extensively for its combination of electrical and thermal conductivity, corrosion resistance, and formability. Unlike steel and aluminum’s heat-treatable grades, pure copper and many of its alloys cannot be hardened by quenching. Their strengthening relies on different mechanisms, which directly determines how welding affects their mechanical properties.

Copper Alloy Group Common Grades Strengthening Mechanism Effect of Welding Weldability
ETP / Pure Copper C11000, C10200 Cold working (work hardening) HAZ fully softened; strength reverts to annealed level Moderate — high preheat required
Brass (Cu-Zn) C26000 (70/30), C36000 Solid solution + work hardening Softened; Zn fuming is a fume hazard Moderate — Zn volatility is a concern
Phosphor Bronze (Cu-Sn) C51000, C54400 Solid solution + work hardening HAZ softened; hot cracking possible if P >0.04% Good
Silicon Bronze (Cu-Si) C65500, C65100 Solid solution + work hardening Good ductility retained; lower preheat needed Very Good
Aluminum Bronze (Cu-Al) C61400, C63000 Solid solution + some phase hardening Risk of HAZ grain boundary oxidation; use GTAW Good with proper procedures
Copper-Nickel (Cu-Ni) C70600 (90/10), C71500 (70/30) Solid solution hardening Moderate strength loss; excellent weld quality achievable Excellent
Beryllium Copper (Cu-Be) C17200, C17500 Precipitation hardening (aging) HAZ over-aged; re-aging required post-weld Limited — Be fume is toxic

Thermal Conductivity: The Dominant Welding Challenge

The single most significant practical challenge when welding copper and most copper alloys is their extremely high thermal conductivity. Pure copper conducts heat at approximately 390 W/m·K — roughly 25 times higher than carbon steel (50 W/m·K) and 60 times higher than austenitic stainless steel (16 W/m·K). The engineering consequence for welding is profound: arc energy is conducted away from the weld pool faster than it can build up sufficient local temperature to achieve fusion.

Comparative Thermal Conductivity of Common Weld Materials: Pure Copper (ETP): ~390 W/m·K // heat sinks heat away rapidly; high preheat mandatory Copper-Nickel 90/10: ~50 W/m·K // similar to carbon steel; lower preheat needed Carbon Steel: ~50 W/m·K // baseline comparison Aluminum (pure): ~235 W/m·K // high conductivity; explains preheat for thicker sections Austenitic SS (316): ~16 W/m·K // low — HAZ steep gradient; keeps heat local // Practical implication: welding 10 mm pure copper requires proportionally // more arc energy than welding 10 mm carbon steel to achieve fusion

Practical consequences of high thermal conductivity in copper welding include:

  • Difficulty establishing the weld pool: Without preheat, the arc energy is dissipated into the surrounding mass, and the weld zone may never reach fusion temperature. Preheat for pure copper sections above 3 mm typically starts at 200 °C and may reach 600 °C for heavy sections.
  • Weld pool fluidity: When fusion is achieved, the liquid copper has very low viscosity compared to steel. It tends to flow out of the joint, particularly in overhead or vertical positions, requiring careful technique and joint design (tight root gaps, backing bars).
  • HAZ width: The high conductivity means the thermal gradient through the HAZ is shallower — the HAZ is wider, and the softened region extends further from the weld centreline than it would for the same heat input in steel.
  • Hydrogen embrittlement (tough-pitch copper): Copper grades containing oxygen (ETP copper — C11000) are susceptible to embrittlement when welded or heated in a reducing atmosphere. Hydrogen from the atmosphere or from the electrode reacts with copper oxide inclusions in the metal to produce steam (H₂O) at grain boundaries, causing intergranular cracking. Always use oxygen-free copper (C10200) or phosphorus-deoxidised copper (C12200) for welded applications, not ETP copper.

Cold-Worked Strength and the Welding Thermal Cycle

Many copper alloys are supplied and used in the cold-worked condition (designations such as 1/4 Hard, 1/2 Hard, Full Hard). Cold working introduces a high density of dislocations into the crystal structure, dramatically increasing strength and hardness above the annealed baseline. A typical 70/30 brass in the full-hard condition has a tensile strength of approximately 600 MPa versus 330 MPa in the fully annealed condition — an 80% increase achieved purely through cold work.

When this material is welded, the HAZ is heated above the recrystallisation temperature of the alloy (typically 250–450 °C for copper alloys depending on composition and degree of cold work). Above this temperature, the cold-worked dislocation structure recovers and the grains recrystallise into a new, coarse-grained, softened structure. This process is irreversible — you cannot restore the cold-worked condition through any post-weld heat treatment short of repeated cold working, which is impossible on a completed weld. The welded joint and adjacent HAZ are permanently at the annealed strength level.

Engineering Design Note: All welded structural joints in cold-worked copper alloys must be designed using the annealed strength values, not the parent material (cold-worked) strength. Joint efficiency in such alloys is calculated against the annealed yield and tensile strength. This is analogous to the strength reduction in heat-treatable aluminum alloys after welding: the design strength at the joint is governed by the HAZ, not the base material.

Precipitation-Hardening Copper Alloys (Beryllium Copper, Chromium Copper)

A small but important subset of copper alloys — principally beryllium copper (Cu-Be) and chromium copper (Cu-Cr) — can be strengthened by an aging heat treatment analogous to the precipitation hardening used for PH stainless steels and 2xxx/7xxx aluminum alloys. In these alloys, the welding thermal cycle dissolves the precipitate structure (solution anneals the HAZ), producing a soft, solution-annealed condition in the weld zone. To restore properties, a post-weld aging heat treatment at 315–480 °C for 2–4 hours is required after welding. Welding engineers specifying procedures for beryllium copper must note that beryllium oxide (BeO) dust and fumes are extremely toxic — mandatory respiratory protection, local exhaust ventilation, and specialist safety procedures are non-negotiable.

Copper-Nickel (CuNi) in Offshore and Marine Applications: Copper-nickel alloys (C70600: 90% Cu / 10% Ni, and C71500: 70% Cu / 30% Ni) are the most commonly welded copper alloys in offshore and marine fabrication — used for seawater piping, condenser tubes, and hull sheathing. Their thermal conductivity is close to that of carbon steel, so welding procedures are more tractable. Use GTAW or GMAW with ERCuNi filler, back-purge the root pass with argon or nitrogen to prevent oxidation, maintain maximum interpass temperature of 100 °C to prevent hot cracking, and avoid iron contamination from carbon steel tooling, which drastically reduces corrosion resistance. See the corrosion guide for CuNi galvanic compatibility data.

Summary Comparison: Three Material Families

Property / Challenge Austenitic Stainless Steel Aluminum Alloys Copper Alloys
Primary HAZ risk Sensitisation / IGC Softening (over-aging or recrystallisation) Softening (recrystallisation)
Hot cracking risk High (control with 4–10 FN) Moderate (Si or Mg fillers required) Low–moderate (high-P grades at risk)
Preheat required? No (except martensitic grades) For sections >6–10 mm typically Yes — often 200–600 °C for pure Cu
PWHT required? Only martensitic grades (temper) Re-aging for precipitation-hardened grades Re-aging for precipitation-hardened grades
Surface preparation Clean; stainless wire brush only Degrease + SS wire brush; oxide reform in <1 s Degrease; remove oxide film
Standard welding process GTAW, GMAW, SMAW (low-H) AC GTAW, GMAW (DCEP) GTAW (DCEN), GMAW, OFW
Key filler standard AWS A5.4, A5.9, A5.11 AWS A5.10 / ASME SFA-5.10 AWS A5.7, A5.6 / ASME SFA-5.7
ASME IX P-Number P-No. 6, 7, 8, 10H P-No. 21–26 P-No. 31–35

Frequently Asked Questions

What is sensitization in stainless steel welding and how is it prevented?
Sensitisation is the precipitation of chromium carbides (Cr₃₂C₆) along austenite grain boundaries when the HAZ is held in the temperature range of approximately 427–871 °C during welding. The chromium-depleted zones adjacent to grain boundaries lose their passive film and become vulnerable to intergranular corrosion (IGA) in service. Prevention methods include: using extra-low carbon grades (304L, 316L with max 0.03% C); using stabilised grades containing titanium (321) or niobium (347) which combine with carbon preferentially; or applying a full solution anneal at 1050–1100 °C followed by rapid water quench to re-dissolve carbides after welding. See the stainless steel weld decay guide for IGC testing per ASTM A262.
What is delta ferrite and why is it important in stainless steel welds?
Delta ferrite is a BCC iron phase retained in the solidified austenitic stainless steel weld metal when the weld composition is balanced toward the ferritic side of the Schaeffler or WRC-1992 diagram. A delta ferrite content of 4–10 FN (Ferrite Number) in the as-deposited weld metal effectively prevents solidification (hot short) cracking by providing grain boundary pathways that absorb low-melting-point impurities and interrupt crack propagation. Delta ferrite is ferromagnetic while austenite is not, allowing measurement with a calibrated magnetic gage (ferritescope). Excessively high ferrite (above ~15 FN) can reduce toughness and corrosion resistance after elevated-temperature service where sigma phase can form. See the delta ferrite importance guide for full WRC-1992 diagram usage.
Why is alternating current (AC) used for TIG welding of aluminum?
Aluminum forms a tenacious aluminum oxide film (Al₂O₃) on its surface almost instantly upon air exposure. This oxide has a melting point of approximately 2049 °C — far above aluminum’s melting point of 660 °C — and will prevent proper fusion if not removed. During AC GTAW, the electrode-positive half-cycle generates cathodic bombardment of the weld pool surface, physically breaking up and dispersing the oxide film (the “cleaning action”). The electrode-negative half-cycle provides the primary arc energy for melting the base metal. Argon shielding gas prevents re-oxidation during welding. DCEN, used for steel GTAW, provides no cleaning action and cannot be used effectively for aluminum. See the GTAW welding guide for full parameter guidance.
What filler metals are used to weld 304 and 316 stainless steel?
For Type 304 stainless steel, the standard matching filler is ER308L (low carbon), which provides adequate corrosion resistance and controls sensitisation in the weld deposit. For Type 316 (molybdenum-bearing), the matching filler is ER316L, which maintains the molybdenum content essential for pitting resistance. The “L” designation limits carbon to 0.03% maximum, reducing sensitisation risk in the deposited weld metal. For high-temperature service where a stabilised deposit is needed, ER347 (niobium-stabilised) may be specified. All filler compositions are selected to deposit weld metal with 4–10 FN delta ferrite per the WRC-1992 diagram to prevent hot cracking. Filler specifications are governed by AWS A5.9 / ASME SFA-5.9 for bare wire and A5.4 / SFA-5.4 for covered electrodes.
What welding challenges are specific to martensitic stainless steels like Grade 410?
Martensitic stainless steels such as Grade 410 and 416 have significant hardenability and form hard, brittle martensite in the HAZ upon cooling after welding, in direct analogy to hardenable carbon steels. HAZ hardness can exceed 400 HV, creating susceptibility to hydrogen-induced cold cracking. Typical requirements include: preheat of 150–260 °C (higher for thicker sections or grades above 0.10% C), controlled maximum interpass temperature of 315 °C, low-hydrogen processes (GTAW or low-hydrogen SMAW with E410 or E309L filler), and post-weld tempering at 650–760 °C to restore ductility and toughness. Do not PWHT in the 370–565 °C range due to temper embrittlement risk. These grades are classified as P-No. 6 under ASME Section IX.
Why does welding reduce the strength of work-hardened copper alloys?
Many copper alloys derive their strength from cold working, which introduces a high dislocation density into the crystal structure. When the HAZ is heated above the recrystallisation temperature of the alloy (typically 250–450 °C for copper alloys), the cold-worked microstructure recovers and recrystallises into a softened, coarse-grained condition, permanently eliminating the dislocation density responsible for the elevated strength. This reduction is irreversible — no post-weld heat treatment can restore cold-worked properties without re-working. Welded joint design in cold-worked copper alloys must therefore use annealed strength values for the joint and HAZ zone.
What preheat is required for welding copper and why?
Copper’s thermal conductivity (approximately 390 W/m·K for pure copper) is roughly 25 times higher than carbon steel. Without preheat, arc energy is dissipated into the surrounding mass faster than it can establish a molten pool, resulting in lack of fusion defects. Preheat for pure copper typically starts at 200 °C for sections above 3 mm and may reach 600 °C for heavy sections. Copper-nickel alloys (90/10, 70/30) have much lower thermal conductivity and require proportionally less preheat, but still benefit from at least 50–100 °C preheat on sections above 10 mm. GTAW with argon shielding and DCEN polarity is the preferred process for precision copper welding.
How does the PREN number relate to stainless steel weld quality?
The Pitting Resistance Equivalent Number (PREN) quantifies a stainless steel’s resistance to pitting corrosion: PREN = %Cr + 3.3 × %Mo + 16 × %N. When welding, dilution between filler and base metal, elemental burn-off, and segregation during solidification can reduce local PREN values in the weld deposit below the base metal level. A weld zone with lower PREN is more susceptible to preferential pitting corrosion — a common failure mode in marine, offshore, and chemical environments. Filler metal selection should produce a weld deposit with PREN equal to or higher than the base material. Use the WeldFabWorld PREN calculator to evaluate material combinations. For duplex stainless steels, the duplex welding guide provides detailed PREN and ferrite control requirements.

Recommended Books on Stainless Steel, Aluminum, and Copper Welding

Welding Metallurgy and Weldability of Stainless Steels — Lippold & Kotecki
The definitive reference on stainless steel welding metallurgy — sensitisation, IGA, hot cracking, delta ferrite, duplex grades, and constitution diagrams. Essential for engineers and inspectors.
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Welding Metallurgy, 3rd Edition — Sindo Kou
University-level text covering stainless steel, aluminum, and copper alloy welding metallurgy in full technical depth. Covers solidification, HAZ transformations, and weldability of each material family.
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Aluminum Welding Handbook — AWS
AWS technical handbook covering aluminum alloy series, filler metal selection per A5.10, AC GTAW procedures, oxide film management, and pre/post-weld treatment guidance for all major aluminum grades.
View on Amazon
Ferrite Number Magnetic Gage for Stainless Steel
Calibrated ferritescope for measuring delta ferrite (Ferrite Number) in austenitic stainless steel weld deposits. Essential inspection tool for verifying hot cracking resistance per AWS A4.2 and ASME Section IX.
View on Amazon

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