Published December 5, 2022
| Version v1.0
Dataset
Open
Solar cycle and long-term trends in the observed peak of the meteor altitude distributions by meteor radars
Authors/Creators
- 1. Department of Physics, Catholic University of America, U.S.A., and ITM Physics Laboratory, NASA Goddard Space Flight Center, U.S.A.
- 2. University Bern, Institute of Applied Physics, Microwave Physics, Bern, Switzerland
- 3. ITM Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt MD, U.S.A.
- 4. Institute for Meteorology, Leipzig University, Germany
- 5. British Antarctic Survey, Cambridge, U.K.
- 6. British Antarctic Survey, Cambridge, U.K./University of Bath, Bath, U.K.
- 7. National Institute for Space Research (INPE), São José dos Campos, SP, Brazil
- 8. National Institute for Space Research (INPE), São José dos Campos, SP, Brazil/China-Brazil Joint Laboratory for Space Weather, NSSC/INPE, São José dos Campos, SP, Brazil
- 9. Department of Physics, Federal University of Campina Grande, Campina Grande, PB, Brazil
- 10. Australian Antarctic Division, Kingston, TAS, Australia
- 11. Swedish Institute of Space Physics (IRF), Kiruna, Sweden
- 12. Tromsø Geophysical Observatory, UiT - The Arctic University of Norway, Tromsø, Norway
- 13. National Institute of Polar Research, Tachikawa, Japan/The Graduate University for Advanced Studies (SOKENDAI), Tokyo, Japan
- 14. Sodankylä Geophysical Observatory, University of Oulu, Finland
- 15. Division of Atmospheric Sciences, Korea Polar Research Institute, Incheon, S. Korea
- 16. Department of Physics and Astronomy, University of Leicester, Leicester, U.K.
Description
The datasets here correspond to a paper by Dawkins et al., “Solar cycle and long-term trends in the observed peak of the meteor altitude distributions by meteor radars”, originally submitted in November 2022.
The following datasets are sufficient to produce Figure 2 and 3 in the main manuscript.
Figure 2:
- Please use the 12 individual files with filenames, “Dawkins_et_al_2022__meteor_peak_altitude__*_data.txt”. Here the asterisk should be replaced by one of the following station abbreviations: CAR, COL, CPa, DAV, KIR, KSS, ROT, SMa, SOD, SVA, TdF, and TRO.
- Each file contains 5 columns: Column 1 is year (from 1999 to 2022), Column 2 is the time series of the annual peak altitude residuals (no units), Column 3 is the corresponding standard error, Column 4 is the multilinear model fit, and Column 5 is the normalized annual solar flux (F10.7) in arbitrary units.
Figure 3:
- Please use “Dawkins_et_al_2022__meteor_peak_altitude_trends.txt”. For ease, a description of the different columns is included within this file.
Files
Dawkins_et_al_2022__meteor_peak_altitude__CAR_data.txt
Files
(11.3 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:dda7647c931432b1033cb7f85f8e4f15
|
747 Bytes | Preview Download |
|
md5:7f0fc7cb5f5503d86caf464e11b87c8a
|
821 Bytes | Preview Download |
|
md5:d8714981ef072d0a4ccab253ff254e7e
|
879 Bytes | Preview Download |
|
md5:d1b503afb054150b4c9fc7b3553c267e
|
841 Bytes | Preview Download |
|
md5:76715a4f3aaddfb7e521c01b0a53e4f8
|
883 Bytes | Preview Download |
|
md5:57979de6062cd592dce95ff46ef0084b
|
810 Bytes | Preview Download |
|
md5:c1da72887e94b2c1abf6f645035ff445
|
803 Bytes | Preview Download |
|
md5:22bca517c33ceb77fce47803e729db8a
|
735 Bytes | Preview Download |
|
md5:0c076a4fb43b85ac864eee5971501ba8
|
809 Bytes | Preview Download |
|
md5:3db1a4282c4b7d57ef98491c367fdaf7
|
904 Bytes | Preview Download |
|
md5:fe30efb2dfdb2493003f9df610b699b3
|
793 Bytes | Preview Download |
|
md5:13b15e9138f17bf32f463ad637e9daab
|
876 Bytes | Preview Download |
|
md5:c42700963852dd037c23707d5682bd5c
|
1.4 kB | Preview Download |