file: OO-README.txt init: May 17 2021 Rob Rutten Deil last: Jul 18 2022 Rob Rutten Deil site: https://robrutten.nl/rrweb/rjr-archive/dircontent.html note: started when writing "Compendium solar spectrum formation" https://robrutten.nl/rrweb/rjr-pubs/2021LingAstRep...2R.pdf @RR: renew = addtree in top, newwebfiles ========================== old to ancient solar files ========================== subdirs atlases = spectrum atlases linelists = line tables and similar tables observations = spectroheliograms etc ppmodels = "standard" plane-parallel solar atmosphere models books = diverse books --------------------------------------------- subdirectory atlases = solar spectrum atlases --------------------------------------------- atlases/vitascollection ======================= solar spectrum atlases collected by Nikola Vitas, as zipped IDL save files unzip and read the *.sav file in IDL with restore,'filename', IDL> help shows the variable names (e.g., wavelength, intensity) file atlases_overview.ods = Vitas' libreoffice description spreadsheet atlases/neckel-intatlas.txt =========================== solar disk-center atlas optical spectrum in absolute intensity units (often called "Neckel atlas" but the FTS data are from Brault & Testerman) ascii txt file 3 columns, 1107963 lines, read with eg IDL readcol.pro 3290.0013000 0.3092120 0.3222460 3290.0051000 0.3094180 0.3222470 ........ 12509.9643000 0.0745340 0.0762120 12509.9824000 0.0745750 0.0762120 first column: wavelength second column: solar disk-center intensity third column: local Labs+Neckel-estimated continuum intensity units wavelength: Angstrom converted to air from wavenumbers sigma = 1/wav_vac with wav_air = 0.99972683 wav_vac + 0.0107 - 196.25/wav_vac corrected by comparison with Pierce & Breckenridge 1973 solar line list so these are solar wavelengths, not laboratory wavelengths intensity: watt / cm2 ster AA as emitted at solar surface (Neckel wrongly specified cm^-1) source made from KPNO McMath FTS scans taken about 1980 by Brault and Testerman same range as NSO-Kurucz flux atlas but absolute disk-center intensity description: Neckel ADS 1999SoPh..184..421N Neckel also offers the corresponding flux = disk-averaged intensity; it is added in Vitas file 1984_Neckel_and_Labs.zip but my file has only disk-center intensity plus continuum estimate. It was used already in Labs+Neckel 1984SoPh...90..205N Continuum: see Neckel ADS 1997SoPh..171..257N gotten per "anonymous ftp" in 1999 at ftp.hs.uni-hamburg.de cd /pub/outgoing/FTS-Atlas check May 17 2021: still present but use lftp to list/get files (Firefox, Chrome etc deprecated ftp links in 2020) IDL program to plot a segment: https://robrutten.nl/rridl/misclib/plotftsint.pro atlases/beckers-fluxatlas.pdf ============================= Scan of the graphical edition of the Sacramento Peak Observatory solar irradiance atlas of Beckers et al. = 1976hrsa.book.....B. ----------------------------------------------------------------------- subsdirectory linelists = solar line wavelength (and intensities) lists ----------------------------------------------------------------------- linelists/MMH.txt ================= Optical spectral line list with equivalent widths published as "The solar spectrum 2935 A to 8770 A" by Moore, Minnaert & Houtgast ADS 1966sst..book.....M. linelists/aq1976.pdf ================ golden oldie also containing line lists linelists/pierce-breckenridge-wavlist.txt ========================================= solar optical line wavelength list from Pierce & Breckenridge ADS 1974kptp.book.....P column content (?) first column seems wavelength in Angstrom, probably air meaning of letter S or T after wavelength? second column ? third column seems wavenumber in cm, possibly vacuum fourth column ? maybe number of spectrograms employed? fifth column ? also letters R. S, M sixth colum = strength? equivalent width? (H&K, Halpha large) seventh = element and ionization stage eighth = multiplet number (likely from MMH) linelists/allende-garcia-wavlist.txt ==================================== Solar optical line wavelengths from Kitt Peak FTS atlases by Allende-Prieto & Garcia Lopex ADS 1998A&AS..131..431A. From both FTS disk-center intensity spectra and flux spectra. linelists/cleanlines-intensity.txt ================================== Solar optical line wavelengths, relative depths, halfwidths, equivalent widths for 750 "clean" lines in the disk-center intensity Jungfraujoch atlas ADS 1973apds.book.....D = Table IV of Rutten & van der Zalm ADS 1984A&AS...55..143R. linelists/cleanlines-flux.txt ============================= Solar optical line wavelengths, relative depths, halfwidths, equivalent widths for 602 "clean" lines in the Sacramento Peak irradiance atlas of Beckers et al. ADS 1976hrsa.book.....B = Table I of Rutten & van der Zalm ADS 1984A&AS...55..171R. linelists/dunnetal-tableIII.txt linelists/dunnetal-redordered.dat linelists/dunnetal-plateheights.dat linelists/dunnetal-bin10AA.png linelists/dunneta-decay.png =================================== Flash-spectrum line intensities from spectrograms taken during the 1962 eclipse by the HAO expedition = Table III etcerea of Dunn et al. ADS 1968ApJS...15..275D. The png files are summary plots. books/1966atp..book.....W.pdf hydrogen through neon books/1969atp..book.....W.pdf sulphur through calcium books/1988JPCRD..17S....F.pdf iron through nickel ============================= NBS (NIST) transition probabilities ----------------------------------- subdirectory observations/KPNO ----------------------------------- Kitt Peak McMath east-auxiliary spectroheliograms received per CD from J.W. Harvey in 2005 = "scans from the photolab" files 10468* taken 1975-09-17 by Bruce Gillespie files 11429* taken 1978-07-14 by Jack Harvey (some wavelength variation over field from uncompensated slit curvature) also one limb spectrum plate taken for Pierce 1968ApJS...17....1P observations/KPNO/10468-2.tif ============================= CaII K2v towards limb often reproduced in different cutouts and orientations, e,g. 1985cdm..proc.....L = Lites SacPeak workshop (cover, negative) 1988assu.book.....Z = Zirin book 1991mcch.conf...48R = Rutten+Uitenbroek Heidelberg proceedings frontispiece to Solar Physics 134 2007ASPC..368...27R = Rutten Coimbra proceedings observations/KPNO/10468-2-pos.jpg ================================= same famous Gillespie K2v heliogram but reversed into positive with sharpness and greyscale optimization observations/KPNO/10468-4.tif ============================= simultaneous with 10468-2.tif but in CN bandhead 3883 AA. observations/KPNO/align_gillespie_ca_cn.idl observations/KPNO/gillespie_ca.fits observations/KPNO/gillespie_cn.fits =================================== 10468-2.tif and 10468-4.tif co-aligned with align_gillespie_ca_cn.idl both positive observations/KPNO/10468-1.tif ============================= looks as CaII K2v center-limb observations/KPNO/10468-3.tif ============================= looks as CN 3883 bandhead observations/KPNO/11429-k3004.jpg ================================= CaII K3 disk center observations/KPNO/11429-k3007.jpg ================================= CaII K3 towards limb observations/KPNO/11429-limbk.jpg ================================= CaII K3 rotated limb cutout of 11429-k3007.jpg observations/KPNO/limbspectrum_4571.png ======================================= limb spectrum for Pierce 1968ApJS...17....1P containing MgI 4571.1 ----------------------------------------- subdirectory observations/Hida ----------------------------------------- Hida emulations of filtergram response from scanning spectrometry = movies with the passband scanning the CaII H&K cores courtesy Satoru UeNo selection from https://www.hida.kyoto-u.ac.jp/DST/spectra/2007/200708/ observations/Hida/armovie.mpg ============================= sampling an active region through the core of CaII H observations/Hida/limbmovie.mpg =============================== sampling a limb scene through the core of CaII K ------------------------------------------------------------------------- subdirectory ppmodels = "standard" plane-parallel solar atmosphere models ------------------------------------------------------------------------- ppmodels/models.txt = 1970s-1980s plane-parallel standard models ================================================================ HSRA # ADS 1971SoPh...18..347G HSRAKIEL # no idea what this is, some Holweger modification? VALIII-A VALIII-B VALIII-C VALIII-D VALIII-E VALIII-F # ADS 1981ApJS...45..635V VALII-M # ADS 1981ApJS...45..635V HOLMUL # ADS 1974SoPh...39...19H LITES # probably Lites thesis ADS 1972PhDT.........7L BELLEA (=THEORETICAL FLUX-CONSTANT LINE BLANKETED LTE MODEL) # ADS 1976A&AS...23...37B VALIII-CEX (= VALIII-C WITH EXTRA INTERPOLATED POINTS) VALIIAYRES (=AYRES MODIFICATION OF VALII-M) # ?? Thomas R. Ayres maybe from ADS 1978SoPh...60...19A? MACKKL (VALIIIC UPDATE MALTBY ET AL., AP.J. JULY 1, 1986) # ADS 1986ApJ...306..284M ppmodels/finemodels.txt = some of the above spline-resampled to 10-km grid ========================================================================== HSRA MACKKL VALIIAYRES HOLMUL LITES BELLEA VALII-M VALIII-C VALIII-A VALIII-B VALIII-D VALIII-E VALIII-F subdirectory ppmodels/RH_Atmos = 1D input models for RH ======================================================= NB: May 24 2021 RH github directory https://github.com/han-uitenbroek/RH/tree/master/Atmos has only the FAL models of ADS 1993ApJ...406..319F. This collection, gotten over the years from Han Uitenbroek, adds more including the models of Fontenla et al. ADS 2009ApJ...707..482F and ALC7 of Avrett & Loeser ADS 2008ApJS..175..229A ------------------------------------------------------------------------- subdirectory books (not digital tables but pdf scans) ------------------------------------------------------------------------- books/rbtsa2013.pdf =================== Raisa Bentsionovna Teplitskaya: Solar Atmosphere, Irkutsk, 2013