|
 |
 |
 |
 |
 |
 |
 |
 |
|
|
|
|
|
|
|
|
|
Space environment domain |
PHOTONS |
PARTICLES |
FIELDS |
||||||
Galactic & Heliospheric |
indices: mu, g_factor | neutral: H, He charged: GCR models: MASTER, ORDEM standards: IS 15390:2004 |
|||||||
Solar |
indices: E10, E81, E1_40, E30_70, E162, Esrc, F10, F81, J_H_I, J_He_I, J_He_II, MgII, M10, M81, Rsn, Rz, S10, S81, XE107, Xb10, Xhf, X10, X81, Y10, Y81 irradiances: I(lambda,t), Lya, Lya_81, Lyman_a_c, 26-34, 1-50, S radiances: 30.4, 28.4, 171.5 systems: SIP PG, SIP SY, APEX(SOHO/SEM), IDAR standards: ISO 21348:2007, ISO DIS 15856, ASTM E490 |
indices: Kp/Ap, Dst charged particles: p, alpha, e models: HAF standards: ISO DIS 15856 |
solar wind: B models: HAF |
||||||
Terrestrial |
aeronomy: Peuv, Qeuv |
|
main magnetic models: IGRF magnetospheric models: A95 standards: ISO DIS 22009 |
||||||
Planetary |
Jupiter: H Saturn: aurora |
Typical uses of the Solar Irradiance Platform:
Indices Key words Typical uses E10, E81, and Ap server solar irradiances satellite drag, electron densities, TEC Solar EUV input for models of the thermosphere and ionosphere; can be used as a substitute for F10.7 in satellite drag analysis and to calculate atmosphere or ionosphere densities. Rsn server solar irradiances amateur radio, HF radio propagation Solar EUV input for ray-trace models; can be used as a substitute for the Wolf sunspot number (Rz) in radio propagation reconstruction and for current or near-term conditions. I(t) server solar irradiances spectral solar irradiances Solar spectral input for first principles models; can also be used to provide up-to-date time variability information for helium and hydrogen solar lines in planetary missions. Peuv server solar irradiances EUV hemisphere power Solar EUV hemispheric power index for comparison with auroral hemispheric power index; can be used to provide up-to-date time variability information for Earth-observing missions. E1_40 server solar irradiances integrated EUV 1-40 nm Solar EUV integrated energy in ergs cm-2 s-1 for comparison with aeronomy-derived values; can be used to provide up-to-date time variability information for Earth-observing missions.