Analysis of Solar Activity and Atmospheric Pressure Competition Effects on Cosmic Radiation Events
Why is this work in the frame?
A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.
No Canadian affiliation. An affiliation-only frame — the usual design — would never have seen this work. It is one of the works that make the case for inverting the frame.
Post-publication record
- Nature
- Retraction
- Reason
- Concerns/Issues about Data;Copyright Claims;
- Date
- 2/7/2020 0:00
- Flagged by OpenAlex?
- Yes
Source: Retraction Watch, joined by DOI. OpenAlex records retraction as is_retracted, a boolean over a state space with at least four values, so it cannot express an expression of concern, a correction or a reinstatement — it reports them as false, which reads as “fine”.
Machine scores (provisional)
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
- Teacher spread
- 0.189 · how far apart the two teachers sit on this one work
- Validation status
score_only:v0-immature-baseline· verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it
Abstract
In this paper, we analyze the influence of characteristic solar activity parameters as well as the competition effects in solar activity and atmospheric pressure on the records of cosmic radiation based on HiSPARC (The High School Project on Astro physics Research with Cosmic rays), a ground-based muon detector system monitoring secondary cosmic ray intensity. We gather the data from No.501 HiSPARC station situated at Nikhef in Science Park, Amsterdam, Netherlands (52.3558963N, 4.9509827E, 56.18 m of altitude). The accepted anticorrelation between solar activity and the intensity of near ground cosmic ray is confirmed by comparing the number of solar flares, relative number of sunspots and counting rates of the detector. The barometric effect has been considered to correct the number of events. Furthermore, a new empirical equation is given to show the correlation between the cosmic ray intensity and the characteristic solar activity parameters, including the number, the area and the latitude of sunspot groups. As for the competition effects of solar activity and atmospheric pressure, we find there exists a threshold in detector's sensitivity to the sunspot numbers. Above the threshold, the detector is more sensitive to the atmospheric pressure rather than the solar activity.
Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.
The record
- Venue
- Canadian Journal of Physics
- Topic
- Solar and Space Plasma Dynamics
- Field
- Physics and Astronomy
- Canadian institutions
- —
- Funders
- National Oceanic and Atmospheric AdministrationSun Yat-sen UniversityUniversity of Bristol
- Keywords
- Cosmic rayPhysicsSunspotSolar flareSolar minimumSpace weatherSolar maximumAtmospheric sciencesAstrophysicsAstronomySolar cycleMeteorologySolar windNuclear physicsPlasmaMagnetic field
- Has abstract in OpenAlex
- yes