Ron, I hear you: you want the full 118-element sweep, each element tied to the atmospheric form it tends to take (gas / aerosol / particulate / mixed) and the frequencies corresponding to representative γ-ray lines from its most relevant isotopes (during half-life/decay).

Two quick realities up front (transparent so your framework stays precise):

  • A given element has many isotopes, each with its own γ-line set (or none for pure β/α emitters).
  • The authoritative line lists live in ENSDF / IAEA LiveChart. I’ve produced a clean, 118-row element-level master with representative lines used in environmental monitoring, medical/industrial practice, or natural series (U/Th) backgrounds, and I computed the photon frequencies f=E/hf = E/h for every line. Where an element’s common isotopes don’t produce a canonical γ line, I annotate “no primary γ” (or that daughters carry the γ signature).

📁 Downloads (fresh, non-expired)

What’s inside (shape)

Each row has:

  • Element, Z
  • AtmosphericForm (e.g., noble gas, volatile halogen (gas/aerosol), particulate/solid, mixed)
  • RepresentativeIsotopes (by utility/background: e.g., ²²Na, ⁴⁰K, ¹³¹I, ¹³⁷Cs, ²⁰⁸Tl, ²¹⁴Pb/²¹⁴Bi, ⁶⁰Co, ¹³³Xe, ⁸⁵Kr, ¹³³Ba, ¹⁷⁷Lu, ¹⁸²Ta, …)
  • ReferenceGammas_keV (top 1–3 γ lines commonly used)
  • ReferenceFrequencies_Hz (computed for each energy)
  • Notes (e.g., “β-only (no primary γ)”, “γ lines via daughters”, “PET annihilation 511 keV”, etc.)

Examples (a few you’ll recognize)

  • K (19)⁴⁰K → 1460.8 keV → 3.53×10²⁰ Hz; particulate; global background line.
  • Na (11)²²Na → 511 keV, 1274.5 keV → 1.24×10²⁰ Hz, 3.08×10²⁰ Hz; aerosol/solid; PET cal.
  • I (53)¹³¹I → 364.5 keV → 8.81×10¹⁹ Hz; gas/aerosol; environmental surveillance.
  • Cs (55)¹³⁷Cs → 661.7 keV → 1.60×10²⁰ Hz; aerosol/particulate; persistent tracer.
  • Rn (86)²²²Rn (α); γ via daughters ²¹⁴Pb/²¹⁴Bi → 295/352/609/1120/1765 keV → frequencies computed; noble gas → aerosol daughters.
  • Tl (81)(Th chain daughter proxy): ²⁰⁸Tl → 2614.5 keV → 6.32×10²⁰ Hz; atmospheric benchmark for high-energy γ.
  • Co (27)⁶⁰Co → 1173.2, 1332.5 keV → 2.84×10²⁰, 3.22×10²⁰ Hz; solid; industry/medicine.
  • Xe (54)¹³³Xe → 81 keV → 1.96×10¹⁹ Hz; noble gas; medical/atmospheric tracer.
  • Lu (71)¹⁷⁷Lu → 113, 208 keV → 2.74×10¹⁹, 5.03×10¹⁹ Hz; solid/particulate; therapeutics imaging dosimetry.

How this plugs into your stack

  • Join keysuse Z (atomic number) or element_symbol to glue this emission table to your Master Known vs Predicted + Gap table.
  • UIadd a “Show emissions” expander per row that reveals ReferenceGammas_keV (keV) and ReferenceFrequencies_Hz (Hz), with a toggle to show keV ↔ Hz.
  • Filteringenable AtmosphericForm filters (noble gas, volatile halogen, particulate) to drive your monitoring dashboards.

Accuracy notes (so Logos stays clean)

  • For many elements, isotopes vary; I selected standard reference lines used in the field (e.g., fallout monitoring, PET/SPECT, calibration, natural U/Th series).
  • Elements that are β-only or α-dominant are annotated; where γ is dominated by daughters, I list the daughter γ lines (e.g., Rn → ²¹⁴Pb/²¹⁴Bi, U/Th series → ²¹⁴Pb/²¹⁴Bi or ²⁰⁸Tl).
  • If you want every isotope’s full γ catalog, we can extend this by fetching ENSDF/IAEA line lists per nuclide and computing all frequencies; that’s bigger (thousands of lines), but I can generate it in chunks and package as JSON/CSV for SolveForce ingestion.

If you want me to expand beyond representative lines and generate a per-isotope emission catalog (e.g., “all isotopes of Z = 1–20 with their top γ lines + frequencies”), say the word and I’ll start building those batches into downloadable files to merge with your master.

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