Automated Author ProfileVictoriya, Forsythe
ASTRA, LLC0000-0003-0894-2951
Victoriya, Forsythe
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets for this author
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the author's datasets
Total Mentions
Total mentions of the author's datasets
S-Index Interpretation
The S-Index (Sharing Index) is a comprehensive metric that represents the cumulative impact of all your datasets. It is calculated as the sum of Dataset Index scores across all your claimed datasets.
What it means:
- A higher S-index indicates greater overall impact of your datasets relative to typical datasets in their fields of research
- The S-Index grows as you add more datasets or as existing datasets gain more citations and mentions
- It provides a single number to track your research data impact over time
Current S-Index: 24.5 (sum of 16 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
A SAMI3 run was performed for June 10, 2025, using constant indices: F10.7 = 124 sfu, F10.7a = 136 sfu, Ap = 4, and Kp = 1.
Authors
- Forsythe, Victoriya
A SAMI3 run was performed for June 10, 2025, using constant indices: F10.7 = 124 sfu, F10.7a = 136 sfu, Ap = 4, and Kp = 1.
Authors
- Forsythe, Victoriya
This is a set of the synthetic tangent points for the radio occultation data used in the OSSE study titled "The analysis of the ionospheric radio occultation data coverage for ANCHOR ionospheric data assimilation". The inc in the title indicates the inclination of the orbit, and the numsat indicates the number of the equally-spaced satellites in that orbit.
Authors
- Forsythe, Victoriya ;
- Gullotta, William
This is a set of the synthetic tangent points for the radio occultation data used in the OSSE study titled "The analysis of the ionospheric radio occultation data coverage for ANCHOR ionospheric data assimilation". The inc in the title indicates the inclination of the orbit, and the numsat indicates the number of the equally-spaced satellites in that orbit.
Authors
- Forsythe, Victoriya ;
- Gullotta, William
Contained are the ISR derived parameters extracted for four events between the years 2018 and 2024 spanning four radars located at Arecibo, Jicamarca, Millstone Hill, and Poker Flat. Parameters are stored in one file per radar per event. The parameters are stored in pickled python files ending in '.pkl'. Each fiile contains the following:PyIRI_NmF2 - Peak electron density of F2 layer from PyIRIPyIRI_hmF2 - Altitde of peak F2 electron density from PyIRIPyIRI_B_bot - The bottom side thickness of the F2 layer from PyIRIPyIRI_B_top - The topside thickness of the F2 layer from PyIRIstime - UT time of the observationnumber - Unique number identifierNmF2 - Peak electron density of F2 layer from observations hmF2 - Altitude of peak F2 electron density from observationsB_top - Bottom side thickness of the F2 layer from observationsB_bot - Topside thickness of the F2 layer from observations
Authors
- Pepper, Andrew ;
- Makarevich, Victoriya
Contained are the ISR derived parameters extracted for four events between the years 2018 and 2024 spanning four radars located at Arecibo, Jicamarca, Millstone Hill, and Poker Flat. Parameters are stored in one file per radar per event. The parameters are stored in pickled python files ending in '.pkl'. Each fiile contains the following:PyIRI_NmF2 - Peak electron density of F2 layer from PyIRIPyIRI_hmF2 - Altitde of peak F2 electron density from PyIRIPyIRI_B_bot - The bottom side thickness of the F2 layer from PyIRIPyIRI_B_top - The topside thickness of the F2 layer from PyIRIstime - UT time of the observationnumber - Unique number identifierNmF2 - Peak electron density of F2 layer from observations hmF2 - Altitude of peak F2 electron density from observationsB_top - Bottom side thickness of the F2 layer from observationsB_bot - Topside thickness of the F2 layer from observations
Authors
- Pepper, Andrew ;
- Makarevich, Victoriya
The data were simulated using the Observation System Simulation Experiment Tool (OSSET). OSEET was developed by ASTRA LLC to provide the Air Force (AF) the capability to perform assessments of the utility of existing and planned sensors for ionospheric specification.
Authors
- Forsythe, Victoriya
The data were simulated using the Observation System Simulation Experiment Tool (OSSET). OSEET was developed by ASTRA LLC to provide the Air Force (AF) the capability to perform assessments of the utility of existing and planned sensors for ionospheric specification.
Authors
- Forsythe, Victoriya
Correlation time (or relaxation parameter) for the ionospheric data assimilation. each .nc file in this folder corresponds to a particular bin. Binning in season: 0=month 1,2,11,12
1=month 5,6,7,8
2=month 3,4,9,10
Binning in F10.7 solar flux: 0=0-100 s.f.u
1=100-200 s.f.u.
2=200-350 s.f.u. Example:
The name of the .nc file:
Corr_Time_season_02_sf_01.nc
would correspond to season with bin 2, solar flux with bin 1. Inside of the .nc files: Mlons=array of geomagnetic longitudes (degrees)
Mlats=array of geomagnetic latitudes (degrees)
corr_time=array of size (nlon, nlat), is a map of correlation times (hours)
Authors
- Forsythe, Victoriya
Correlation time (or relaxation parameter) for the ionospheric data assimilation. each .nc file in this folder corresponds to a particular bin. Binning in season: 0=month 1,2,11,12
1=month 5,6,7,8
2=month 3,4,9,10
Binning in F10.7 solar flux: 0=0-100 s.f.u
1=100-200 s.f.u.
2=200-350 s.f.u. Example:
The name of the .nc file:
Corr_Time_season_02_sf_01.nc
would correspond to season with bin 2, solar flux with bin 1. Inside of the .nc files: Mlons=array of geomagnetic longitudes (degrees)
Mlats=array of geomagnetic latitudes (degrees)
corr_time=array of size (nlon, nlat), is a map of correlation times (hours)
Authors
- Forsythe, Victoriya