Rules of the Road
SuperMAG is made possible by the generous contribution by a long list of collaborators. To ensure their continued operation the user must follow the below rules-of-the-road.
Data, plots or derived data products are provided under the limitations of "fair use" and cannot be redistributed. Contact the individual instrument PI and the SuperMAG PI for requests that are in conflict with these restrictions.
The user is requested to acknowledge individual collaborators and SuperMAG when original data, derived data, movies, or data products are used in publications and/or presentations.
In all cases:
- Include acknowledgement as listed on the SuperMAG website.
- Include references to a technical papers for stations used.
- Include SuperMAG reference: Gjerloev, J. W. (2012), The SuperMAG data processing technique, J. Geophys. Res., 117, A09213, doi:10.1029/2012JA017683.
In cases that a few stations play a key role and their data are central to the scientific conclusion of the paper:
- Offer of co-authorship to the PI (or PIs) of those stations.
For the ground magnetometer data we gratefully acknowledge:
Intermagnet; USGS, Jeffrey J. Love; CARISMA, PI Ian Mann; CANMOS;
The S-RAMP Database, PI K. Yumoto and Dr. K. Shiokawa; The SPIDR
database; AARI, PI Oleg Troshichev; The MACCS program, PI
M. Engebretson, Geomagnetism Unit of the Geological Survey of
Canada; GIMA; MEASURE, UCLA IGPP and Florida Institute of
Technology; SAMBA, PI Eftyhia Zesta; 210 Chain, PI K. Yumoto;
SAMNET, PI Farideh Honary; The institutes who maintain the IMAGE
magnetometer array, PI Eija Tanskanen; PENGUIN; AUTUMN, PI Martin
Connors; DTU Space, PI Dr. Rico Behlke; South Pole and McMurdo
Magnetometer, PI's Louis J. Lanzarotti and Alan T. Weatherwax;
ICESTAR; RAPIDMAG; PENGUIn; British Artarctic Survey; McMac, PI
Dr. Peter Chi; BGS, PI Dr. Susan Macmillan; Pushkov Institute of
Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
(IZMIRAN); GFZ, PI Dr. Juergen Matzka; MFGI, PI B. Heilig; IGFPAS,
PI J. Reda; University of L’Aquila, PI M. Vellante; BCMT, V. Lesur
and A. Chambodut; Data obtained in cooperation with Geoscience
Australia, PI Marina Costelloe; SuperMAG, PI Jesper W. Gjerloev.
Lichtenberger J., M. Clilverd, B. Heilig, M. Vellante, J. Manninen, C. Rodger, A. Collier, A. Jørgensen, J. Reda, R. Holzworth, and R. Friedel (2013), The plasmasphere during a space weather event: first results from the PLASMON project, J. Space Weather Space Clim., 3, A23 (www.swsc-journal.org/articles/swsc/pdf/2013/01/swsc120062.pdf).
Tanskanen, E.I. (2009), A comprehensive high-throughput analysis of substorms observed by IMAGE magnetometer network: Years 1993-2003 examined, 114, A05204, doi:10.1029/2008JA013682.
Engebretson, M. J., W. J. Hughes, J. L. Alford, E. Zesta, L. J. Cahill, Jr., R. L. Arnoldy, and G. D. Reeves (1995), Magnetometer array for cusp and cleft studies observations of the spatial extent of broadband ULF magnetic pulsations at cusp/cleft latitudes , J. Geophys. Res., 100, 19371-19386, doi:10.1029/95JA00768.
Chi, P. J., M. J. Engebretson, M. B. Moldwin, C. T. Russell, I. R. Mann, M. R. Hairston, M. Reno, J. Goldstein, L. I. Winkler, J. L. Cruz-Abeyro, D.-H. Lee, K.Yumoto, R. Dalrymple, B. Chen, and J. P. Gibson (2013), Sounding of the plasmasphere by Mid-continent MAgnetoseismic Chain magnetometers, J. Geophys. Res. Space Physics, 118, doi:10.1002/jgra.50274.
MAGDAS / 210 Chain:
Yumoto, K,. and the CPMN Group (2001), Characteristics of Pi 2 magnetic pulsations observed at the CPMN stations: A review of the STEP results, Earth Planets Space, 53, 981-992.
Gjerloev, J. W. (2012), The SuperMAG data processing technique, J. Geophys. Res., 117 , A09213, doi:10.1029/2012JA017683.