J/ApJS/210/12           Solar photoionization rates           (Bochsler+, 2014)

Solar photoionization rates for interstellar neutrals in the inner heliosphere: H, He, O, and Ne. Bochsler P., Kucharek H., Mobius E., Bzowski M., Sokol J.M., Didkovsky L., Wieman S. <Astrophys. J. Suppl. Ser., 210, 12 (2014)> =2014ApJS..210...12B 2014ApJS..210...12B
ADC_Keywords: Atomic physics ; Interstellar medium ; Sun ; Ultraviolet Keywords: atomic processes; ISM: atoms; Sun: heliosphere; Sun: UV radiation Abstract: Extreme UV (EUV) spectra from the Thermosphere Ionosphere Mesosphere Energetics and Dynamics (TIMED)/Solar EUV Experiment are used to infer photoionization rates in the inner heliosphere. Relating these rates to various proxies describing the solar EUV radiation, we construct a multi-linear model which allows us to extrapolate ionization rates back to periods when no routine measurements of the solar EUV spectral distribution have been available. Such information is important, e.g., for comparing conditions of the interstellar neutral particles in the inner heliosphere at the time of Ulysses/GAS observations with conditions during the more recent observations of the Interstellar Boundary Explorer. From a period of 11 yr when detailed spectra from both TIMED and three proxies -- Solar and Heliospheric Observatory/CELIAS/SEM-rates, F10.7 radio flux, and Mg II core-to-wing indices -- have been available, we conclude that the simple model is able to reproduce the photoionization rates with an uncertainty of typically 5%. Description: Using the spectral data for solar extreme UV (EUV) routinely available from Thermosphere Ionosphere Mesosphere Energetics and Dynamics/Solar EUV Experiment (TIMED/SEE), we have derived the photoionization rates of H, He, O, and Ne at the location of the Earth for the period from the launch of TIMED in 2002 up through the end of 2012. We compared these rates with a set of three proxies, count rates from the Solar Extreme Ultraviolet Monitor (SEM) on the Charge, ELement, and Isotope Analysis System (CELIAS) of the Solar and Heliospheric Observatory (SOHO) spacecraft, the F10.7 cm radio flux, and the MgII core-to-wing index. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 87 51978 Photoionization rates for H, He, O, and Ne at the location of the Earth table2.dat 49 12210 Adjusted radio-flux rates -------------------------------------------------------------------------------- See also: J/ApJ/717/674 : Ionization energies of CnN(n=4-12) (Kostko+, 2010) J/ApJ/707/482 : Models of the solar atmosphere. III. (Fontenla+, 2009) J/ApJ/667/1119 : Photoionization of H in strong magnetic fields (Zhao+, 2007) J/A+A/439/387 : Absolute photoionization cross sections (Bizau+, 2005) J/A+A/432/1063 : Analysis of inner solar corona in EUV (Lanzafame+, 2005) J/A+A/422/337 : Solar EUV Post-Eruptive Arcades (Tripathi+, 2004) J/ApJ/543/1016 : EUV spectrum of solar active region (Brosius+ 2000) J/A+AS/113/237 : Ultraviolet Spectrum of the Sun (Samain, 1995) J/ApJS/91/461 : EUV spectrum of solar active region (Thomas+, 1994) http://www.usc.edu/dept/space_science/sem_data/downloadSEM.html : SEM data http://lasp.colorado.edu/see/see_data.html : TIMED/SEE web site Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Num [1/255] Spectrum index number 5- 8 I4 yr Obs.Y [2002/2012] Year of the observation 10- 12 I3 d Obs.D [1/366] Day of the year of the observation 14- 20 F7.1 s Start Start time 22- 28 F7.1 s End End time 30- 39 F10.5 yr Year [2002/2013] Fractional year time 41- 51 E11.5 s-1 HRate [5.4e-8/1.9e-7] H photoionization rate 53- 63 E11.5 s-1 HeRate [4.1e-8/1.9e-7] He photoionization rate 65- 75 E11.5 s-1 ORate [1.8e-7/7.1e-7] O photoionization rate 77- 87 E11.5 s-1 NeRate [1.2e-7/7.1e-7] Ne photoionization rate -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 yr Obs.Y [1978/2012] Year of the observation 6- 8 I3 d Obs.D [1/366] Day of the year of the observation 10- 17 F8.3 yr Year [1978/2013] Fractional year time 19- 25 F7.5 10-7/s HRate [0.73/1.2] H photoionization rate 27- 33 F7.5 10-7/s HeRate [0.77/1.6] He photoionization rate 35- 41 F7.5 10-7/s ORate [0.79/1.4] O photoionization rate 43- 49 F7.5 10-7/s NeRate [0.78/1.8] Ne photoionization rate -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 28-Jan-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line