On the public citation graph

Corona Holes in Low Latitude May Not Be the Origin of Streams and of 27-Day Recurrent Geomagnetic Storms

https://doi.org/10.2139/ssrn.4051360
0 signed · 16 inferred · view as graph

Inferred edges come from two machine sources: sweeps of open repository metadata (mostly SSRN and Zenodo), and a bulk OpenAlex citation snapshot. Every row below is labelled with the one it came from. Neither is a complete citation index — absence here is not evidence of absence.

Is this your work? Sign in with ORCID and put your name on the claims that are yours.
Claim with ORCID
Reference health. See whether every reference in this work resolves to a known work and none has been retracted — and get a dated CiteStamped badge you can embed.
See reference health

What this work says

Outgoing claims: the papers this work cites, builds on, or argues with.

inferredcites →https://doi.org/10.1007/bf00349000openalex-extracted
Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms
inferredcites →https://doi.org/10.1007/s11207-018-1348-8openalex-extracted
High-Speed Solar Wind Streams and Geomagnetic Storms During Solar Cycle 24
inferredcites →https://doi.org/10.1007/s11214-005-8052-3openalex-extracted
A New Morphology of Solar Activity and Recurrent Geomagnetic Disturbances: The Late-Declining Phase of the Sunspot Cycle
inferredcites →https://doi.org/10.1007/s12036-015-9338-9openalex-extracted
Solar Wind Associated with Near Equatorial Coronal Hole
inferredcites →https://doi.org/10.1016/0032-0633(88)90068-2openalex-extracted
Quantitative forecasting of the 27-day recurrent magnetic activity
inferredcites →https://doi.org/10.1016/j.jastp.2019.02.007openalex-extracted
On the explosive nature of auroral substorms and solar flares: The electric current approach
inferredcites →https://doi.org/10.1029/2018ja026005openalex-extracted
Nine Outstanding Questions of Solar Wind Physics
inferredcites →https://doi.org/10.1029/gm002p0001openalex-extracted
Solar-Terrestrial Relationship
inferredcites →https://doi.org/10.1029/ja092ia05p04339openalex-extracted
Three‐dimensional structure of the coronal magnetic field and the solar wind speed distribution projected on the photosphere in 1974
inferredcites →https://doi.org/10.1029/ja094ia05p05453openalex-extracted
The sunspot cycle variations of the neutral line on the source surface
inferredcites →https://doi.org/10.1088/0004-637x/714/2/1672openalex-extracted
FORMATION OF CORONAL HOLES ON THE ASHES OF ACTIVE REGIONS
inferredcites →https://doi.org/10.1088/0004-637x/775/2/100openalex-extracted
LOW-LATITUDE CORONAL HOLES, DECAYING ACTIVE REGIONS, AND GLOBAL CORONAL MAGNETIC STRUCTURE
inferredcites →https://doi.org/10.1088/0004-637x/779/1/2openalex-extracted
WEAKEST SOLAR WIND OF THE SPACE AGE AND THE CURRENT “MINI” SOLAR MAXIMUM
inferredcites →https://doi.org/10.1134/s001679320904001xopenalex-extracted
Studying correlations between the coronal hole area, solar wind velocity, and local magnetic indices in the Canadian region during the decline phase of cycle 23
inferredcites →https://doi.org/10.3847/1538-4357/aa7de4openalex-extracted
Exploring the Inner Acceleration Region of Solar Wind: A Study Based on Coronagraphic UV and Visible Light Data
inferredcites →https://doi.org/10.3847/1538-4357/aac8e3openalex-extracted
The Highly Structured Outer Solar Corona
Editorial review for independent work. ICSAC — the Institute for Complexity Science and Advanced Computing — runs a structured editorial panel for researchers publishing outside journals, and publishes on CiteStamp rails. Submission is free and goes through ORCID: icsacinstitute.org/submit.