orphans of abductivism: Superposed epoch analyses and statistical functions for IMF, Solar corona, Solar wind, magnetosphere, and ionosphere records (SuperMAG, NASA, NOAA, etc.) embedded with LIGO event (N=11) source luminosity distance and radiated energy with respect to day and 5-min window of trigger arrival

Time domain histograms (superposed epoch analyses) and statistical functions for solar, IMF/solar wind, magnetosphere, and ionosphere records for complete available datasets (SuperMAG, NASA, NOAA, etc.). y=event counts, with daily LIGO events (N=11), embedded, with y=luminosity distance as calculated by LIGO.

[Under construction continuing 2019-05013, to be updated to incorporate N=20 events and N=44 rejected triggers from combined O1,O2,O3 LIGO-Virgo event catalogs/reports]

data sources for these analyses:

https://solarflare.njit.edu/dataproducts.html
http://www.sidc.be/silso/groupnumberv3
https://www.ngdc.noaa.gov/stp/satellite/goes/dataaccess.html
ftp://ftp.ncdc.noaa.gov/pub/data/swdi/database-csv/v2/
https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/tgf/
http://www.solen.info/solar/coronal_holes.html
http://supermag.jhuapl.edu/substorms/
https://www.ligo.org/detections/

1. Sunspot-free days, daily counts, sample period 1849-2017; LIGO N=11 GW events, day/yr, luminosity distance; 2. Sunspot-free days, daily counts, sample period 1849-2017; LIGO N=11 GW events, energy radiated:

1.Sunspot-free days, counts, sample period 1849-2017; LIGO N=11 GW events; N=43 reported false triggers, day; 2. Sunspot-free days, counts, year beginning June 21; LIGO GW events, day/yr, luminosity distance:

1. Sunspots, zero and all Fibonacci number daily counts, sample period 1849-2017; LIGO N=11 GW events, luminosity distance|day; 2. Sunspot-free and Fibonacci SS# days, counts, year beginning June 21; LIGO GW events, day/yr, luminosity distance :

SSN 3-day intervals centered on LIGO trigger days, SSN change; scatter distributions of degenerate LIGO parameters; tabulated statistics:

Earth-facing coronal holes, interval boundary days; LIGO GW events, day, luminosity distance [to be updated]:

1. Solar proton events, daily counts/yr; LIGO GW events, day/yr, luminosity distance [to be updated]; solar proton events, 5-minute counts, 24-hours UTC; 2. LIGO GW event counts, 5-min bins/day, luminosity distance [to be updated]:

Fermi solar flares, daily counts/yr; LIGO GW events, daily/yr:

1. Fermi TGF triggers (terrestrial gamma ray flashes), daily counts/yr; LIGO GW events, day/yr, luminosity distance [to be updated]; 2. Fermi TGF triggers (terrestrial gamma ray flashes), 5-min counts 24-hours UTC; LIGO GW events, count triggers 5-min/day bins [to be updated]: