J/A+A/655/A51       Solar evolutionary and structure models    (Kunitomo+, 2021)

Imprint of planet formation in the deep interior of the Sun. Kunitomo M., Guillot T. <Astron. Astrophys. 655, A51 (2021)> =2021A&A...655A..51K 2021A&A...655A..51K (SIMBAD/NED BibCode)
ADC_Keywords: Sun ; Models, evolutionary ; Abundances ; Stars, pre-main sequence Keywords: Sun: abundances - Sun: interior - stars: protostars - stars: pre-main sequence - accretion, accretion disks - planets and satellites: formation Abstract: In protoplanetary disks, the growth and inward drift of dust lead to the generation of a temporal "pebble wave" of increased metallicity. This phase must be followed by a phase in which the exhaustion of the pebbles in the disk and the formation of planets lead to the accretion of metal-poor gas. At the same time, disk winds may lead to the selective removal of hydrogen and helium from the disk. Hence, stars grow by accreting gas that has an evolving composition. In this work, we investigated how the formation of the Solar System may have affected the composition and structure of the Sun, and whether it plays any role in solving the so-called solar-abundance problem, that is, the fact that standard models with up-to-date lower-metallicity abundances reproduce helioseismic constraints significantly more poorly than those with old higher-metallicity abundances. We simulated the evolution of the Sun from the protostellar phase to the present age and attempted to reproduce spectroscopic and helioseismic constraints. We performed chi-squared tests to optimize our input parameters, which we extended by adding secondary parameters. These additional parameters accounted for the variations in the composition of the accreted material and an increase in the opacities. We confirmed that, for realistic models, planet formation occurs when the solar convective zone is still massive; thus, the overall changes due to planet formation are too small to significantly improve the chi-square fits. We found that solar models with up-to-date abundances require an opacity increase of 12% to 18% centered at T=106.4K to reproduce the available observational constraints. This is slightly higher than, but is qualitatively in good agreement with, recent measurements of higher Fe opacities. These models result in better fits to the observations than those using old abundances; therefore, they are a promising solution to the solar abundance problem. Using these improved models, we found that planet formation processes leave a small imprint in the solar core, whose metallicity is enhanced by up to 5%. This result can be tested by accurately measuring the solar neutrino flux. In the improved models, the protosolar molecular cloud core is characterized by a primordial metallicity in the range Zproto=0.0127-0.0157 and a helium mass fraction in the range Yproto=0.268-0.274. Description: File tablea contains the input parameters and results of 65 solar models optimized using chi-squared simulations. The structure and evolution data of the optimized cases of models K2-A2-12, K2-MZ5, and K23-MZvar-A2-12 are also provided. The stellar evolution code MESA version 12115 was used. See also https://doi.org/10.5281/zenodo.5372058 File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea.dat 822 65 Results of 65 solar models (tables A1-A2) prof/* . 3 Individual files of stellar structure of models K2-A2-12, K2-MZ5 and K23-MZvar-A2-12 at the solar age hist/* . 3 Indivudal files of evolution of models K2-A2-12, K2-MZ5 and K23-MZvar-A2-1 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- Name Model name 21- 42 E22.17 --- alphaMLT Mixing-length parameter 44- 65 E22.17 --- fovershoot Overshooting parameter 67- 74 F8.6 --- Xproto Primordial hydrogen abundance (mass fraction) 76- 97 E22.17 --- Yproto Primordial helium abundance 99-120 E22.17 --- Zproto Primordial metallicity 122-143 E22.18 --- Zaccmax Maximum accretion metallicity 145-166 E22.17 Msun M1 Stellar mass when Zacc starts to increase 168-189 E22.17 Msun M2 Stellar mass when Zacc decreases to zero 191-193 F3.1 --- A1 Opacity enhancement parameter at logT=5.66 195-216 E22.17 --- A2 Opacity enhancement parameter at logT=6.45 218-240 E23.17 --- A3 Opacity enhancement parameter at logT=7.18 242-263 E22.17 --- Yaccmin Minimum helium abundance of accretion gas 265-268 F4.1 Myr tacc Accretion timescale 270-291 E22.17 --- chi2 Chi-square value 293-314 E22.17 --- csrms Root mean square of sound speed at 4.567Gyr 316-337 E22.17 --- ZXsurf Ratio of the surface metallicity to the surface hydrogen abundance at 4.567Gyr 339-360 E22.17 --- Ysurf Surface helium abundance at 4.567Gyr 362-383 E22.17 Rsun Rcz Location of the convective-radiative boundary 385-407 E23.17 [Lsun] logL log(bolometric luminosity) at 4.567Gyr 409-430 E22.17 K Teff Effective temperature at 4.567Gyr 432-454 E23.17 --- Zcenter Central metallicity at 4.567Gyr 456-475 F20.18 --- Zsurf Surface metallicity at 4.567Gyr 477-498 E22.19 Msun MXYlost Mass ejected from the disk assuming MZ,planet=150M{earth} 500-520 F21.16 Mgeo MZplanet Metal mass retained by planets assuming MXY,lost=0 522-544 E23.17 K Tcenter Central temperature at 4.567Gyr 546-568 E23.17 10-7J/cm3 Pcenter Central pressure at 4.567Gyr (erg/cm3) 570-587 F18.14 g/cm3 rhocenter Central density at 4.567Gyr 589-611 E23.17 --- Xcenter Central hydrogen abundance at 4.567Gyr 613-635 E23.17 --- Ycenter Central helium abundance at 4.567Gyr 637-659 E23.17 --- mucenter Central mean molecular weight at 4.567Gyr 661-678 F18.16 cm2/g kapcenter Central opacity at 4.567Gyr 680-702 E23.17 1/cm2.s Phipp pp neutrino flux at the Earth at 4.567Gyr 704-726 E23.17 1/cm2.s Phipep pep neutrino flux at the Earth at 4.567Gyr 728-750 E23.17 1/cm2.s Phi7Be 7Be neutrino flux at the Earth at 4.567Gyr 752-774 E23.17 1/cm2.s Phi8B 8B neutrino flux at the Earth at 4.567Gyr 776-798 E23.17 1/cm2.s PhiN13 N13 neutrino flux at the Earth at 4.567Gyr 800-822 E23.17 1/cm2.s PhiO15 O15 neutrino flux at the Earth at 4.567Gyr -------------------------------------------------------------------------------- Description of file: Byte-by-byte Description of file (#): prof/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 40 I40 --- zone Zone 58- 81 E24.17 K logT log(temperature) 99- 122 E24.17 [g/cm3] logRho log(density) 140- 163 E24.17 [10-7J/cm3] logP log(pressure) 181- 204 E24.17 --- logR logR 222- 245 E24.17 [Lsun] luminosity Luminosity 263- 286 E24.17 --- eps_grav eps_grav 304- 327 E24.17 --- signedlogeps_grav signedlogeps_grav 345- 368 E24.17 --- net_energy net_energy 386- 409 E24.17 --- signedlogpower signedlogpower 427- 450 E24.17 --- velocity velocity 468- 491 E24.17 --- entropy Entropy, in kB/u unit, kB is the Boltzmann constant and u is the unified atomic mass unit 509- 532 E24.17 --- mixing_type mixing_type 550- 573 E24.17 cm/s csound Sound speed at cell center 591- 614 E24.17 --- csound_face csound_face 632- 655 E24.17 --- vdivcsound vdivcsound 673- 696 E24.17 --- eta eta 714- 737 E24.17 --- mu Mean molecular weight 755- 778 E24.17 --- logdq logdq 796- 819 E24.17 --- dq_ratio dq_ratio 837- 860 E24.17 --- q q 878- 901 E24.17 Rsun radius Radius 919- 942 E24.17 --- rmid rmid 960- 983 E24.17 --- rdivR rdivR 1001-1024 E24.17 --- temperature temperature 1042-1065 E24.17 --- tau tau 1083-1106 E24.17 --- logtau logtau 1124-1147 E24.17 --- pressure pressure 1165-1188 E24.17 --- pgasdivptotal pgasdivptotal 1206-1229 E24.17 --- logPgas pgasdivptotal 1247-1270 E24.17 --- logE logE 1288-1311 E24.17 --- grada grada 1329-1352 E24.17 --- dE_dRho dE_dRho 1370-1393 E24.17 --- cv cv 1411-1434 E24.17 --- cp cp 1452-1475 E24.17 --- logS logS 1493-1516 E24.17 --- gamma1 gamma1 1534-1557 E24.17 --- gamma3 gamma3 1575-1598 E24.17 --- logfree_e logfree_e 1616-1639 E24.17 --- chiRho chiRho 1657-1680 E24.17 --- chiT chiT 1698-1721 E24.17 --- abar abar 1739-1762 E24.17 --- zbar zbar 1780-1803 E24.17 --- ye ye 1821-1844 E24.17 [cm2/g] log_opacity log(opacity) 1862-1885 E24.17 --- eps_nuc eps_nuc 1903-1926 E24.17 --- nonnucneu nonnucneu 1944-1967 E24.17 --- mltmixinglength mltmixinglength 1985-2008 E24.17 --- mltmixingtype mltmixingtype 2026-2049 E24.17 --- gradTsubgrada gradTsubgrada 2067-2090 E24.17 --- logDmix logDmix 2108-2131 E24.17 --- logconvvel logconvvel 2149-2172 E24.17 --- convveldiv_csound convveldiv_csound 2190-2213 E24.17 --- logmltD_mix logmltD_mix 2231-2254 E24.17 --- pressurescaleheight pressurescaleheight 2272-2295 E24.17 --- gradT gradT 2313-2336 E24.17 --- gradr gradr 2354-2377 E24.17 --- dlnd_dt dlnd_dt 2395-2418 E24.17 --- dlnT_dt dlnT_dt 2436-2459 E24.17 --- signed_dlnd signed_dlnd 2477-2500 E24.17 --- signed_dlnT signed_dlnT 2518-2541 E24.17 Msun mass Mass coordinate 2559-2582 E24.17 --- m_grav m_grav 2600-2623 E24.17 --- mgravdivmbaryonic mgravdivmbaryonic 2641-2664 E24.17 --- masscorrectionfactor masscorrectionfactor 2682-2705 E24.17 --- logxq logxq 2723-2746 E24.17 --- logxm logxm 2764-2787 E24.17 --- x Hydrogen mass fraction 2805-2828 E24.17 --- y Helium mass fraction 2846-2869 E24.17 --- z Metallicity 2887-2910 E24.17 --- h1 H1 2928-2951 E24.17 --- h2 H2 2969-2992 E24.17 --- he3 He3 3010-3033 E24.17 --- he4 He4 3051-3074 E24.17 --- li7 Li7 3092-3115 E24.17 --- be7 Be7 3133-3156 E24.17 --- b8 B8 3174-3197 E24.17 --- c12 C12 3215-3238 E24.17 --- c13 C13 3256-3279 E24.17 --- n13 N13 3297-3320 E24.17 --- n14 N14 3338-3361 E24.17 --- n15 N15 3379-3402 E24.17 --- o14 O14 3420-3443 E24.17 --- o15 O15 3461-3484 E24.17 --- o16 O16 3502-3525 E24.17 --- o17 O17 3543-3566 E24.17 --- o18 O17 3584-3607 E24.17 --- f17 F17 3625-3648 E24.17 --- f18 F18 3666-3689 E24.17 --- f19 F19 3707-3730 E24.17 --- ne18 Ne18 3748-3771 E24.17 --- ne19 Ne19 3789-3812 E24.17 --- ne20 Ne20 3830-3853 E24.17 --- mg22 Mg22 3871-3894 E24.17 --- mg24 Mg24 3912-3935 E24.17 --- h1-2 H1 3953-3976 E24.17 --- he3-2 He3 3994-4017 E24.17 --- he4-2 He4 4035-4058 E24.17 --- pp pp 4076-4099 E24.17 --- cno cno 4117-4140 E24.17 --- tri_alfa tri_alfa 4158-4181 E24.17 --- burn_c C burn 4199-4222 E24.17 --- burn_n N burn 4240-4263 E24.17 --- burn_o O burn 4281-4304 E24.17 --- burn_ne Ne burn 4322-4345 E24.17 --- burn_na Na burn 4363-4386 E24.17 --- burn_mg Mg burn 4404-4427 E24.17 --- burn_si Si burn 4445-4468 E24.17 --- burn_s S burn 4486-4509 E24.17 --- burn_ar Ar burn 4527-4550 E24.17 --- burn_ca Ca burn 4568-4591 E24.17 --- burn_ti Ti burn 4609-4632 E24.17 --- burn_cr Cr burn 4650-4673 E24.17 --- burn_fe Fe burn 4691-4714 E24.17 --- c12_c12 c12_c12 4732-4755 E24.17 --- c12_o16 c12_o16 4773-4796 E24.17 --- o16_o16 o16_o16 4814-4837 E24.17 --- pnhe4 pnhe4 4855-4878 E24.17 --- photo photo 4896-4919 E24.17 --- ni56_co56 ni56_co56 4937-4960 E24.17 --- co56_fe56 co56_fe56 4978-5001 E24.17 --- other other 5019-5042 E24.17 --- edv_h1 edv_h1 5060-5083 E24.17 --- edv_he3 edv_he3 5101-5124 E24.17 --- edv_he4 edv_he4 5142-5165 E24.17 --- edv_o16 edv_o16 5183-5206 E24.17 --- edv_mg24 edv_mg24 5224-5247 E24.17 --- csatcell_bdy csatcell_bdy -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): hist/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 40 I40 --- model_number Model number 58- 81 E24.17 yr star_age Stellar Age 99- 122 E24.17 Msun star_mass Stellar mass 140- 163 E24.17 Msun/yr star_mdot Stellar accretion rate 181- 204 E24.17 --- time_step time_step 222- 245 E24.17 --- num_zones num_zones 263- 286 E24.17 --- massconvcore massconvcore 304- 327 E24.17 --- convmx1top Bottom of the largest convective region by mass in Mstar unit 345- 368 E24.17 --- convmx1bot Top of the 2nd largest convective region by mass in Mstar unit 386- 409 E24.17 --- convmx2top Top of the 2nd largest convective region by mass in Mstar unit 427- 450 E24.17 --- convmx2bot Bottom of the 2nd largest convective region by mass in Mstar unit 468- 491 E24.17 --- mx1_top mx1_top 509- 532 E24.17 --- mx1_bot mx1_bot 550- 573 E24.17 --- mx2_top mx2_top 591- 614 E24.17 --- mx2_bot mx2_bot 632- 655 E24.17 --- convmx1top_r convmx1top_r 673- 696 E24.17 --- convmx1bot_r convmx1bot_r 714- 737 E24.17 --- convmx2top_r convmx2top_r 755- 778 E24.17 --- convmx2bot_r convmx2bot_r 796- 819 E24.17 --- mx1topr mx1topr 837- 860 E24.17 --- mx1botr mx1botr 878- 901 E24.17 --- mx2topr mx2topr 919- 942 E24.17 --- mx2botr mx2botr 960- 983 E24.17 --- epsnucM1 epsnucM1 1001- 1024 E24.17 --- epsnucM2 epsnucM2 1042- 1065 E24.17 --- epsnucM3 epsnucM3 1083- 1106 E24.17 --- epsnucM4 epsnucM4 1124- 1147 E24.17 --- epsnucM5 epsnucM5 1165- 1188 E24.17 --- epsnucM6 epsnucM6 1206- 1229 E24.17 --- epsnucM7 epsnucM7 1247- 1270 E24.17 --- epsnucM8 epsnucM8 1288- 1311 E24.17 --- hecoremass He core mass 1329- 1352 E24.17 --- ccoremass C core mass 1370- 1393 E24.17 --- ocoremass O core mass 1411- 1434 E24.17 --- sicoremas Si core masss 1452- 1475 E24.17 --- fecoremass Fe core mass 1493- 1516 E24.17 --- neutronrichcore_mass Neutrino rich core mass 1534- 1557 E24.17 --- dynamic_timescale Dynamic time scale 1575- 1598 E24.17 --- kh_timescale kh time scale 1616- 1639 E24.17 --- mdot_timescale Mdot time scale 1657- 1680 E24.17 --- log_LH log(LH) 1698- 1721 E24.17 --- log_LHe log(LHe) 1739- 1762 E24.17 --- log_LZ log(LZ) 1780- 1803 E24.17 --- log_Lnuc log(Lnuc) 1821- 1844 E24.17 --- logLnucsublogL logLnucsublogL 1862- 1885 E24.17 --- extra_L extra_L 1903- 1926 E24.17 --- logextraL logextraL 1944- 1967 E24.17 --- log_Lneu log_Lneu 1985- 2008 E24.17 --- epsgravintegral epsgravintegral 2026- 2049 E24.17 --- logabsLgrav logabsLgrav 2067- 2090 E24.17 K log_Teff log(effective temperature) 2108- 2131 E24.17 --- photosphere_L photosphere_L 2149- 2172 E24.17 --- photosphere_r photosphere_r 2190- 2213 E24.17 --- luminosity Luminosity 2231- 2254 E24.17 [Lsun] log_L log(bolometric luminosity) 2272- 2295 E24.17 [Rsun] log_R log(R) 2313- 2336 E24.17 --- radius Stellar radius 2354- 2377 E24.17 [cm/s2] log_g Surface gravity 2395- 2418 E24.17 --- gravity Gravity 2436- 2459 E24.17 --- photospherecelllog_opacity 2477- 2500 E24.17 --- photospherecelllog_density 2518- 2541 E24.17 --- logsurfcell_pressure 2559- 2582 E24.17 --- surfaceopticaldepth Surface optical depth 2600- 2623 E24.17 --- surfavgomega Surface average omega 2641- 2664 E24.17 [K] logcenterT log(central temperature) 2682- 2705 E24.17 pg/cm3] logcenterRho log(central density) 2723- 2746 E24.17 --- logcenterP log(central P) 2764- 2787 E24.17 --- center_degeneracy Central degeneracy 2805- 2828 E24.17 --- center_mu Central mu 2846- 2869 E24.17 --- center_ye Central ye 2887- 2910 E24.17 --- center_abar Central abar 2928- 2951 E24.17 --- center_entropy Central ntropy 2969- 2992 E24.17 --- center_h1 Central H1 3010- 3033 E24.17 --- center_h2 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7766- 7789 E24.17 --- mixqtop37 mixqtop37 7807- 7830 E24.17 --- mixtype38 mixtype38 7848- 7871 E24.17 --- mixqtop38 mixqtop38 7889- 7912 E24.17 --- mixtype39 mixtype39 7930- 7953 E24.17 --- mixqtop39 mixqtop39 7971- 7994 E24.17 --- mixtype40 mixtype40 8012- 8035 E24.17 --- mixqtop40 mixqtop40 8053- 8076 E24.17 --- mixtype41 mixtype41 8094- 8117 E24.17 --- mixqtop41 mixqtop41 8135- 8158 E24.17 --- mixtype42 mixtype42 8176- 8199 E24.17 --- mixqtop42 mixqtop42 8217- 8240 E24.17 --- mixtype43 mixtype43 8258- 8281 E24.17 --- mixqtop43 mixqtop43 8299- 8322 E24.17 --- mixtype44 mixtype44 8340- 8363 E24.17 --- mixqtop44 mixqtop44 8381- 8404 E24.17 --- mixtype45 mixtype45 8422- 8445 E24.17 --- mixqtop45 mixqtop45 8463- 8486 E24.17 --- mixtype46 mixtype46 8504- 8527 E24.17 --- mixqtop46 mixqtop46 8545- 8568 E24.17 --- mixtype47 mixtype47 8586- 8609 E24.17 --- mixqtop47 mixqtop47 8627- 8650 E24.17 --- mixtype48 mixtype48 8668- 8691 E24.17 --- mixqtop48 mixqtop48 8709- 8732 E24.17 --- mixtype49 mixtype49 8750- 8773 E24.17 --- mixqtop49 mixqtop49 8791- 8814 E24.17 --- mixtype50 mixtype50 8832- 8855 E24.17 --- mixqtop50 mixqtop50 8873- 8896 E24.17 --- mixtype51 mixtype51 8914- 8937 E24.17 --- mixqtop51 mixqtop51 8955- 8978 E24.17 --- mixtype52 mixtype52 8996- 9019 E24.17 --- mixqtop52 mixqtop52 9037- 9060 E24.17 --- mixtype53 mixtype53 9078- 9101 E24.17 --- mixqtop53 mixqtop53 9119- 9142 E24.17 --- mixtype54 mixtype54 9160- 9183 E24.17 --- mixqtop54 mixqtop54 9201- 9224 E24.17 --- mixtype55 mixtype55 9242- 9265 E24.17 --- mixqtop55 mixqtop55 9283- 9306 E24.17 --- mixtype56 mixtype56 9324- 9347 E24.17 --- mixqtop56 mixqtop56 9365- 9388 E24.17 --- mixtype57 mixtype57 9406- 9429 E24.17 --- mixqtop57 mixqtop57 9447- 9470 E24.17 --- mixtype58 mixtype58 9488- 9511 E24.17 --- mixqtop58 mixqtop58 9529- 9552 E24.17 --- mixtype59 mixtype59 9570- 9593 E24.17 --- mixqtop59 mixqtop59 9611- 9634 E24.17 --- mixtype60 mixtype60 9652- 9675 E24.17 --- mixqtop60 mixqtop60 9693- 9716 E24.17 --- mixtype61 mixtype61 9734- 9757 E24.17 --- mixqtop61 mixqtop61 9775- 9798 E24.17 --- mixtype62 mixtype62 9816- 9839 E24.17 --- mixqtop62 mixqtop62 9857- 9880 E24.17 --- mixtype63 mixtype63 9898- 9921 E24.17 --- mixqtop63 mixqtop63 9939- 9962 E24.17 --- mixtype64 mixtype64 9980-10003 E24.17 --- mixqtop64 mixqtop64 10021-10044 E24.17 --- mixtype65 mixtype65 10062-10085 E24.17 --- mixqtop65 mixqtop65 10103-10126 E24.17 --- mixtype66 mixtype66 10144-10167 E24.17 --- mixqtop66 mixqtop66 10185-10208 E24.17 --- mixtype67 mixtype67 10226-10249 E24.17 --- mixqtop67 mixqtop67 10267-10290 E24.17 --- mixtype68 mixtype68 10308-10331 E24.17 --- mixqtop68 mixqtop68 10349-10372 E24.17 --- mixtype69 mixtype69 10390-10413 E24.17 --- mixqtop69 mixqtop69 10431-10454 E24.17 --- mixtype70 mixtype70 10472-10495 E24.17 --- mixqtop70 mixqtop70 10513-10536 E24.17 --- mixtype71 mixtype71 10554-10577 E24.17 --- mixqtop71 mixqtop71 10595-10618 E24.17 --- mixtype72 mixtype72 10636-10659 E24.17 --- mixqtop72 mixqtop72 10677-10700 E24.17 --- mixtype73 mixtype73 10718-10741 E24.17 --- mixqtop73 mixqtop73 10759-10782 E24.17 --- mixtype74 mixtype74 10800-10823 E24.17 --- mixqtop74 mixqtop74 10841-10864 E24.17 --- mixtype75 mixtype75 10882-10905 E24.17 --- mixqtop75 mixqtop75 10923-10946 E24.17 --- mixtype76 mixtype76 10964-10987 E24.17 --- mixqtop76 mixqtop76 11005-11028 E24.17 --- mixtype77 mixtype77 11046-11069 E24.17 --- mixqtop77 mixqtop77 11087-11110 E24.17 --- mixtype78 mixtype78 11128-11151 E24.17 --- mixqtop78 mixqtop78 11169-11192 E24.17 --- mixtype79 mixtype79 11210-11233 E24.17 --- mixqtop79 mixqtop79 11251-11274 E24.17 --- mixtype80 mixtype80 11292-11315 E24.17 --- mixqtop80 mixqtop80 11333-11356 E24.17 --- burntype1 burntype1 11374-11397 E24.17 --- burnqtop1 burnqtop1 11415-11438 E24.17 --- burntype2 burntype2 11456-11479 E24.17 --- burnqtop2 burnqtop2 11497-11520 E24.17 --- burntype3 burntype3 11538-11561 E24.17 --- burnqtop3 burnqtop3 11579-11602 E24.17 --- burntype4 burntype4 11620-11643 E24.17 --- burnqtop4 burnqtop4 11661-11684 E24.17 --- burntype5 burntype5 11702-11725 E24.17 --- burnqtop5 burnqtop5 11743-11766 E24.17 --- burntype6 burntype6 11784-11807 E24.17 --- burnqtop6 burnqtop6 11825-11848 E24.17 --- burntype7 burntype7 11866-11889 E24.17 --- burnqtop7 burnqtop7 11907-11930 E24.17 --- burntype8 burntype8 11948-11971 E24.17 --- burnqtop8 burnqtop8 11989-12012 E24.17 --- burntype9 burntype9 12030-12053 E24.17 --- burnqtop9 burnqtop9 12071-12094 E24.17 --- burntype10 burntype10 12112-12135 E24.17 --- burnqtop10 burnqtop10 12153-12176 E24.17 --- burntype11 burntype11 12194-12217 E24.17 --- burnqtop11 burnqtop11 12235-12258 E24.17 --- burntype12 burntype12 12276-12299 E24.17 --- burnqtop12 burnqtop12 12317-12340 E24.17 --- burntype13 burntype13 12358-12381 E24.17 --- burnqtop13 burnqtop13 12399-12422 E24.17 --- burntype14 burntype14 12440-12463 E24.17 --- burnqtop14 burnqtop14 12481-12504 E24.17 --- burntype15 burntype15 12522-12545 E24.17 --- burnqtop15 burnqtop15 12563-12586 E24.17 --- burntype16 burntype16 12604-12627 E24.17 --- burnqtop16 burnqtop16 12645-12668 E24.17 --- burntype17 burntype17 12686-12709 E24.17 --- burnqtop17 burnqtop17 12727-12750 E24.17 --- burntype18 burntype18 12768-12791 E24.17 --- burnqtop18 burnqtop18 12809-12832 E24.17 --- burntype19 burntype19 12850-12873 E24.17 --- burnqtop19 burnqtop19 12891-12914 E24.17 --- burntype20 burntype20 12932-12955 E24.17 --- burnqtop20 burnqtop20 12973-12996 E24.17 --- burntype21 burntype21 13014-13037 E24.17 --- burnqtop21 burnqtop21 13055-13078 E24.17 --- burntype22 burntype22 13096-13119 E24.17 --- burnqtop22 burnqtop22 13137-13160 E24.17 --- burntype23 burntype23 13178-13201 E24.17 --- burnqtop23 burnqtop23 13219-13242 E24.17 --- burntype24 burntype24 13260-13283 E24.17 --- burnqtop24 burnqtop24 13301-13324 E24.17 --- burntype25 burntype25 13342-13365 E24.17 --- burnqtop25 burnqtop25 13383-13406 E24.17 --- burntype26 burntype26 13424-13447 E24.17 --- burnqtop26 burnqtop26 13465-13488 E24.17 --- burntype27 burntype27 13506-13529 E24.17 --- burnqtop27 burnqtop27 13547-13570 E24.17 --- burntype28 burntype28 13588-13611 E24.17 --- burnqtop28 burnqtop28 13629-13652 E24.17 --- burntype29 burntype29 13670-13693 E24.17 --- burnqtop29 burnqtop29 13711-13734 E24.17 --- burntype30 burntype30 13752-13775 E24.17 --- burnqtop30 burnqtop30 13793-13816 E24.17 --- burntype31 burntype31 13834-13857 E24.17 --- burnqtop31 burnqtop31 13875-13898 E24.17 --- burntype32 burntype32 13916-13939 E24.17 --- burnqtop32 burnqtop32 13957-13980 E24.17 --- burntype33 burntype33 13998-14021 E24.17 --- burnqtop33 burnqtop33 14039-14062 E24.17 --- burntype34 burntype34 14080-14103 E24.17 --- burnqtop34 burnqtop34 14121-14144 E24.17 --- burntype35 burntype35 14162-14185 E24.17 --- burnqtop35 burnqtop35 14203-14226 E24.17 --- burntype36 burntype36 14244-14267 E24.17 --- burnqtop36 burnqtop36 14285-14308 E24.17 --- burntype37 burntype37 14326-14349 E24.17 --- burnqtop37 burnqtop37 14367-14390 E24.17 --- burntype38 burntype38 14408-14431 E24.17 --- burnqtop38 burnqtop38 14449-14472 E24.17 --- burntype39 burntype39 14490-14513 E24.17 --- burnqtop39 burnqtop39 14531-14554 E24.17 --- burntype40 burntype40 14572-14595 E24.17 --- burnqtop40 burnqtop40 14613-14636 E24.17 --- burntype41 burntype41 14654-14677 E24.17 --- burnqtop41 burnqtop41 14695-14718 E24.17 --- burntype42 burntype42 14736-14759 E24.17 --- burnqtop42 burnqtop42 14777-14800 E24.17 --- burntype43 burntype43 14818-14841 E24.17 --- burnqtop43 burnqtop43 14859-14882 E24.17 --- burntype44 burntype44 14900-14923 E24.17 --- burnqtop44 burnqtop44 14941-14964 E24.17 --- burntype45 burntype45 14982-15005 E24.17 --- burnqtop45 burnqtop45 15023-15046 E24.17 --- burntype46 burntype46 15064-15087 E24.17 --- burnqtop46 burnqtop46 15105-15128 E24.17 --- burntype47 burntype47 15146-15169 E24.17 --- burnqtop47 burnqtop47 15187-15210 E24.17 --- burntype48 burntype48 15228-15251 E24.17 --- burnqtop48 burnqtop48 15269-15292 E24.17 --- burntype49 burntype49 15310-15333 E24.17 --- burnqtop49 burnqtop49 15351-15374 E24.17 --- burntype50 burntype50 15392-15415 E24.17 --- burnqtop50 burnqtop50 15433-15456 E24.17 --- burntype51 burntype51 15474-15497 E24.17 --- burnqtop51 burnqtop51 15515-15538 E24.17 --- burntype52 burntype52 15556-15579 E24.17 --- burnqtop52 burnqtop52 15597-15620 E24.17 --- burntype53 burntype53 15638-15661 E24.17 --- burnqtop53 burnqtop53 15679-15702 E24.17 --- burntype54 burntype54 15720-15743 E24.17 --- burnqtop54 burnqtop54 15761-15784 E24.17 --- burntype55 burntype55 15802-15825 E24.17 --- burnqtop55 burnqtop55 15843-15866 E24.17 --- burntype56 burntype56 15884-15907 E24.17 --- burnqtop56 burnqtop56 15925-15948 E24.17 --- burntype57 burntype57 15966-15989 E24.17 --- burnqtop57 burnqtop57 16007-16030 E24.17 --- burntype58 burntype58 16048-16071 E24.17 --- burnqtop58 burnqtop58 16089-16112 E24.17 --- burntype59 burntype59 16130-16153 E24.17 --- burnqtop59 burnqtop59 16171-16194 E24.17 --- burntype60 burntype60 16212-16235 E24.17 --- burnqtop60 burnqtop60 16253-16276 E24.17 --- burntype61 burntype61 16294-16317 E24.17 --- burnqtop61 burnqtop61 16335-16358 E24.17 --- burntype62 burntype62 16376-16399 E24.17 --- burnqtop62 burnqtop62 16417-16440 E24.17 --- burntype63 burntype63 16458-16481 E24.17 --- burnqtop63 burnqtop63 16499-16522 E24.17 --- burntype64 burntype64 16540-16563 E24.17 --- burnqtop64 burnqtop64 16581-16604 E24.17 --- burntype65 burntype65 16622-16645 E24.17 --- burnqtop65 burnqtop65 16663-16686 E24.17 --- burntype66 burntype66 16704-16727 E24.17 --- burnqtop66 burnqtop66 16745-16768 E24.17 --- burntype67 burntype67 16786-16809 E24.17 --- burnqtop67 burnqtop67 16827-16850 E24.17 --- burntype68 burntype68 16868-16891 E24.17 --- burnqtop68 burnqtop68 16909-16932 E24.17 --- burntype69 burntype69 16950-16973 E24.17 --- burnqtop69 burnqtop69 16991-17014 E24.17 --- burntype70 burntype70 17032-17055 E24.17 --- burnqtop70 burnqtop70 17073-17096 E24.17 --- burntype71 burntype71 17114-17137 E24.17 --- burnqtop71 burnqtop71 17155-17178 E24.17 --- burntype72 burntype72 17196-17219 E24.17 --- burnqtop72 burnqtop72 17237-17260 E24.17 --- burntype73 burntype73 17278-17301 E24.17 --- burnqtop73 burnqtop73 17319-17342 E24.17 --- burntype74 burntype74 17360-17383 E24.17 --- burnqtop74 burnqtop74 17401-17424 E24.17 --- burntype75 burntype75 17442-17465 E24.17 --- burnqtop75 burnqtop75 17483-17506 E24.17 --- burntype76 burntype76 17524-17547 E24.17 --- burnqtop76 burnqtop76 17565-17588 E24.17 --- burntype77 burntype77 17606-17629 E24.17 --- burnqtop77 burnqtop77 17647-17670 E24.17 --- burntype78 burntype78 17688-17711 E24.17 --- burnqtop78 burnqtop78 17729-17752 E24.17 --- burntype79 burntype79 17770-17793 E24.17 --- burnqtop79 burnqtop79 17811-17834 E24.17 --- burntype80 burntype80 17852-17875 E24.17 --- burnqtop80 burnqtop80 17893-17916 E24.17 [1/cm2/s] totr_pp1 pp neutrino flux at the Earth 17934-17957 E24.17 [1/cm2/s] totr_pep2 pep neutrino flux at the Earth 17975-17998 E24.17 [1/cm2/s] totrbe7wk_li7 7Be neutrino flux at the Earth 18016-18039 E24.17 [1/cm2/s] totrb8decay 8B neutrino flux at the Earth 18057-18080 E24.17 [1/cm2/s] totrn13decay N13 neutrino flux at the Earth 18098-18121 E24.17 [1/cm2/s] totro15decay O15 neutrino flux at the Earth 18139-18162 E24.17 --- nonnucneu_plas nonnucneu_plas 18180-18203 E24.17 --- nonnucneu_brem nonnucneu_brem 18221-18244 E24.17 --- nonnucneu_phot nonnucneu_phot 18262-18285 E24.17 --- nonnucneu_pair nonnucneu_pair 18303-18326 E24.17 --- nonnucneu_reco nonnucneu_reco -------------------------------------------------------------------------------- Acknowledgements: Masanobu Kunitomo, kunitomo.masanobu(at)gmail.com
(End) Patricia Vannier [CDS] 03-Sep-2021
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