Articles | Volume 44, issue 2
https://doi.org/10.5194/angeo-44-811-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-44-811-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
High latitude, dayside rapid geomagnetic variations observed with ground-based magnetometers in Greenland
Marie Vigger Eldor
CORRESPONDING AUTHOR
Division of Geomagnetism and Geospace, DTU Space, National Space Institute, Technical University of Denmark, Akademivej 356, 2800 Kgs. Lyngby, Denmark
Tromsø Geophysical Observatory (TGO), UiT the Arctic University of Norway, 9037 Tromsø, Norway
Magnar Gullikstad Johnsen
Tromsø Geophysical Observatory (TGO), UiT the Arctic University of Norway, 9037 Tromsø, Norway
Nils Olsen
Division of Geomagnetism and Geospace, DTU Space, National Space Institute, Technical University of Denmark, Akademivej 356, 2800 Kgs. Lyngby, Denmark
Anna Naemi Willer
Division of Geomagnetism and Geospace, DTU Space, National Space Institute, Technical University of Denmark, Akademivej 356, 2800 Kgs. Lyngby, Denmark
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Cited articles
Banks, P. M., Chappell, C. R., and Nagy, A. F.: A new model for the interaction of auroral electrons with the atmosphere: Spectral degradation, backscatter, optical emission, and ionization, J. Geophys. Res., 79, 1459–1470, https://doi.org/10.1029/JA079i010p01459, 1974. a, b
Bartels, J.: Annals of The International Geophysical Year, Vol. 4,, chap. 4, The technique of scaling indices K and Q of geomagnetic activity, Pergamon Press, London, New York, Paris, 215–226, https://doi.org/10.1016/B978-1-4832-1304-0.50006-3, 1957. a
Brekke, A., Feder, T., and Berger, S.: Pc4 giant pulsations recorded in Tromso, 1929–1985, J. Atmos. Terr. Phys., 49, 1027–1032, https://doi.org/10.1016/0021-9169(87)90109-7, 1987. a
Elphic, R. C., Lockwood, M., Cowley, S. W. H., and Sandholt, P. E.: Flux transfer events at the magnetopause and in the ionosphere, Geophys. Res. Lett., 17, 2241–2244, https://doi.org/10.1029/gl017i012p02241, 1990. a
Engebretson, M. J., Hughes, W. J., Alford, J. L., Zesta, E., Cahill, L. J., Arnoldy, R. L., and Reeves, G. D.: Magnetometer array for cusp and cleft studies observations of the spatial extent of broadband ULF magnetic pulsations at cusp/cleft latitudes, J. Geophys. Res.-Space, 100, 19 371–19 386, https://doi.org/10.1029/95ja00768, 1995. a, b, c, d
Engebretson, M. J., Posch, J. L., Pilipenko, V. A., and Chugunova, O. M.: ULF waves at very high latitudes, American Geophysical Union, 137–156, https://doi.org/10.1029/169gm10, 2006. a
Eschenhagen, M.: On minute, rapid, periodic changes of the Earth’s magnetism, Terrestrial Magnetism, 2, 105–114, https://doi.org/10.1029/tm002i003p00105, 1897. a
Feldstein, Y. and Starkov, G.: Dynamics of auroral belt and polar geomagnetic disturbances, Planet. Space Sci., 15, 209–229, https://doi.org/10.1016/0032-0633(67)90190-0, 1967. a
Friis-Christensen, E. and Wilhjelm, J.: Polar cap currents for different directions of the interplanetary magnetic field in the Y-Z plane, J. Geophys. Res., 80, 1248–1260, https://doi.org/10.1029/ja080i010p01248, 1975. a, b
Friis-Christensen, E., McHenry, M. A., Clauer, C. R., and Vennerstrøm, S.: Ionospheric traveling convection vortices observed near the polar cleft: A triggered response to sudden changes in the solar wind, Geophys. Res. Lett., 15, 253–256, https://doi.org/10.1029/gl015i003p00253, 1988. a, b
Fuselier, S. A., Kletzing, C. A., Petrinec, S. M., Trattner, K. J., George, D., Bounds, S. R., Sawyer, R. P., Bonnell, J. W., Burch, J. L., Giles, B. L., and Strangeway, R. J.: Multiple Reconnection X-Lines at the Magnetopause and Overlapping Cusp Ion Injections, J. Geophys. Res.-Space, 127, e30354, https://doi.org/10.1029/2022JA030354, 2022. a
Glassmeier, K. H.: ULF pulsations in the polar cusp and cap, in: Electromagnetic Coupling in the Polar Clefts and Caps, edited by: Sandholt, P. E. and Egeland, A., 167 pp., https://doi.org/10.1007/978-94-009-0979-3_12, 1989. a
Greenstadt, E. W., Inouye, G. T., Green, I. M., and Judge, D. L.: Vela 3 magnetograms at 18 RE structure and pulsations in the magnetosheath, J. Geophys. Res., 72, 3855–3876, https://doi.org/10.1029/jz072i015p03855, 1967. a
Harang, L.: Observations of micropulsations in the magnetic records at Tromsø, Terrestrial Magnetism and Atmospheric Electricity, 37, 57, https://doi.org/10.1029/TE037i001p00057, 1932. a
Hasegawa, H., Wang, J., Dunlop, M. W., Pu, Z. Y., Zhang, Q. H., Lavraud, B., Taylor, M. G. G. T., Constantinescu, O. D., Berchem, J., Angelopoulos, V., McFadden, J. P., Frey, H. U., Panov, E. V., Volwerk, M., and Bogdanova, Y. V.: Evidence for a flux transfer event generated by multiple X-line reconnection at the magnetopause, Geophys. Res. Lett., 37, L16101, https://doi.org/10.1029/2010GL044219, 2010. a
Heppner, J. P., Sugiura, M., Skillman, T. L., Ledley, B. G., and Campbell, M.: OGO-A magnetic field observations, J. Geophys. Res., 72, 5417–5471, https://doi.org/10.1029/jz072i021p05417, 1967. a
Holzworth, R. H. and Meng, C.: Mathematical representation of the auroral oval, Geophys. Res. Lett., 2, 377–380, https://doi.org/10.1029/gl002i009p00377, 1975. a
Jacobs, J. A.: Geomagnetic micropulsations, vol. 1, Springer Verlag, https://doi.org/10.1007/978-3-642-86828-3, 1970. a
Jacobs, J. A., Kato, Y., Matsushita, S., and Troitskaya, V. A.: Classification of geomagnetic micropulsations, J. Geophys. Res., 69, 180–181, https://doi.org/10.1029/jz069i001p00180, 1964. a, b
Johnsen, M. G. and Lorentzen, D. A.: A statistical analysis of the optical dayside open/closed field line boundary, J. Geophys. Res.-Space, 117, https://doi.org/10.1029/2011ja016984, 2012. a, b
Kepko, L. and Kivelson, M.: Generation of Pi2 pulsations by bursty bulk flows, J. Geophys. Res.-Space, 104, 25021–25034, https://doi.org/10.1029/1999ja900361, 1999. a
Kozyreva, O., Pilipenko, V., Lorentzen, D., Baddeley, L., and Hartinger, M.: Transient Oscillations Near the Dayside Open‐Closed Boundary: Evidence of Magnetopause Surface Mode?, J. Geophys. Res.-Space, 124, 9058–9074, https://doi.org/10.1029/2018ja025684, 2019. a
Lee, L. C., Shi, Y., and Lanzerotti, L. J.: A mechanism for the generation of cusp region hydromagnetic waves, J. Geophys. Res., 93, 7578–7585, https://doi.org/10.1029/JA093iA07p07578, 1988. a
Lester, M., Hughes, J. W., and Singer, H. J.: Polarization patterns of Pi 2 magnetic pulsations and the substorm current wedge, J. Geophys. Res.-Space, 88, 7958–7966, https://doi.org/10.1029/ja088ia10p07958, 1983. a
Lockwood, M. and Wild, M. N.: On the quasi-periodic nature of magnetopause flux transfer events, J. Geophys. Res., 98, 5935–5940, https://doi.org/10.1029/92JA02375, 1993. a
Mantas, G. P. and Walker, J. C.: The penetration of soft electrons into the ionosphere, Planet. Space Sci., 24, 409–423, https://doi.org/10.1016/0032-0633(76)90085-4, 1976. a, b
Matzka, J., Bronkalla, O., Tornow, K., Elger, K., and Stolle, C.: Geomagnetic Kp index, https://doi.org/10.5880/KP.0001, 2021a. a
Matzka, J., Stolle, C., Yamazaki, Y., Bronkalla, O., and Morschhauser, A.: The Geomagnetic Kp Index and Derived Indices of Geomagnetic Activity, Space Weather, 19, https://doi.org/10.1029/2020sw002641, 2021b. a
McHarg, M. G. and Olson, J. V.: Correlated optical and ULF magnetic observations of the winter cusp – Boundary layer system, Geophysical Res. Lett., 19, 817–820, https://doi.org/10.1029/92gl00117, 1992. a
McHarg, M. G., Olson, J. V., and Newell, P. T.: ULF cusp pulsations: Diurnal variations and interplanetary magnetic field correlations with ground‐based observations, J. Geophys. Res.-Space, 100, 19729–19742, https://doi.org/10.1029/94ja03054, 1995. a, b
Moen, J. and Brekke, A.: The solar flux influence on quiet time conductances in the auroral ionosphere, Geophys. Res. Lett., 20, 971–974, https://doi.org/10.1029/92gl02109, 1993. a, b
Motoba, T., Ebihara, Y., Ogawa, Y., Kadokura, A., Engebretson, M. J., Angelopoulos, V., Gerrard, A. J., and Weatherwax, A. T.: On the Driver of Daytime Pc3 Auroral Pulsations, Geophys. Res. Lett., 46, 553–561, https://doi.org/10.1029/2018gl080842, 2019. a, b, c
Newell, P. T. and Meng, C.: The cusp and the cleft/boundary layer: Low‐altitude identification and statistical local time variation, J. Geophys. Res.-Space, 93, 14549–14556, https://doi.org/10.1029/ja093ia12p14549, 1988. a
Newell, P. T. and Meng, C.-I.: Dipole tilt angle effects on the latitude of the cusp and cleft/low-latitude boundary layer, J. Geophys. Res.-Space, 94, 6949–6953, https://doi.org/10.1029/JA094iA06p06949, 1989. a, b
Newell, P. T., Meng, C., Sibeck, D. G., and Lepping, R.: Some low‐altitude cusp dependencies on the interplanetary magnetic field, J. Geophys. Res.-Space, 94, 8921–8927, https://doi.org/10.1029/ja094ia07p08921, 1989. a
Newell, P. T., Ruohoniemi, J. M., and Meng, C.: Maps of precipitation by source region, binned by IMF, with inertial convection streamlines, J. Geophys. Res.-Space , 109, https://doi.org/10.1029/2004ja010499, 2004. a, b
Pilipenko, V., Belakhovsky, V., Engebretson, M. J., Kozlovsky, A., and Yeoman, T.: Are dayside long-period pulsations related to the cusp?, Ann. Geophys., 33, 395–404, https://doi.org/10.5194/angeo-33-395-2015, 2015. a, b, c
Pinnock, M., Rodger, A. S., Dudeney, J. R., Baker, K. B., Newell, P. T., Greenwald, R. A., and Greenspan, M. E.: Observations of an enhanced convection channel in the cusp ionosphere, J. Geophys. Res., 98, 3767–3776, https://doi.org/10.1029/92JA01382, 1993. a
Richmond, A. D.: Ionospheric Electrodynamics Using Magnetic Apex Coordinates, J. Geomagn. Geoelectr., 47, 191–212, https://doi.org/10.5636/jgg.47.191, 1995. a
Rinne, Y., Moen, J., Oksavik, K., and Carlson, H. C.: Reversed flow events in the winter cusp ionosphere observed by the European Incoherent Scatter (EISCAT) Svalbard radar, J. Geophys. Res.-Space, 112, A10313, https://doi.org/10.1029/2007JA012366, 2007. a
Rolf, B.: Giant micropulsations at Abisko, Terrestrial Magnetism and Atmospheric Electricity, 36, 9, https://doi.org/10.1029/TE036i001p00009, 1931. a
Rostoker, G., Samson, J. C., and Higuchi, Y.: Occurrence of Pc 4, 5 micropulsation activity at the polar cusp, J. Geophys. Res., 77, 4700–4706, https://doi.org/10.1029/JA077i025p04700, 1972. a, b, c
Russell, C. T. and Elphic, R. C.: Initial ISEE Magnetometer Results: Magnetopause Observations, Space Sci. Rev., 22, 681–715, https://doi.org/10.1007/BF00212619, 1978. a
Russell, C. T. and Elphic, R. C.: ISEE observations of flux transfer events at the dayside magnetopause, Geophys. Res. Lett., 6, 33–36, https://doi.org/10.1029/gl006i001p00033, 1979. a
Sakurai, T. and McPherron, R. L.: Satellite observations of Pi 2 activity at synchronous orbit, J. Geophys. Res.-Space, 88, 7015–7027, https://doi.org/10.1029/ja088ia09p07015, 1983. a, b
Samson, J. C., Harrold, B. G., Ruohoniemi, J. M., Greenwald, R. A., and Walker, A. D. M.: Field line resonances associated with MHD waveguides in the magnetosphere, Geophys. Res. Lett., 19, 441–444, https://doi.org/10.1029/92gl00116, 1992. a
Sandholt, P. E. and Farrugia, C. J.: On the dynamic cusp aurora and IMF By, J. Geophys. Res.-Space, 104, 12461–12472, https://doi.org/10.1029/1999ja900126, 1999. a, b
Sonett, C. P., Judge, D. L., and Kelso, J. M.: Evidence concerning instabilities of the distant geomagnetic field: Pioneer I, J. Geophys. Res., 64, 941–943, https://doi.org/10.1029/jz064i008p00941, 1959. a
Sonnerup, B. U. Ö., Cahill, L. J., and Davis, L. R.: Resonant vibration of the magnetosphere observed from Explorer 26, J. Geophys. Res., 74, 2276–2288, https://doi.org/10.1029/ja074i009p02276, 1969. a
Stauning, P.: Investigations of ionospheric radio wave absorption processes using imaging riometer techniques, J. Atmos. Terr. Phy., 58, 753–764, https://doi.org/10.1016/0021-9169(95)00072-0, 1996. a
Stauning, P.: Polar convection-related ionospheric radiowave absorption processes observed by imaging riometers, Adv. Space Res., 22, 1279–1288, https://doi.org/10.1016/S0273-1177(98)00172-0, 1998. a
Takahashi, K. and Liou, K.: Longitudinal structure of low-latitude Pi2 pulsations and its dependence on aurora, J. Geophys. Res.-Space, 109, A12206, https://doi.org/10.1029/2004JA010580, 2004. a
Vennerstrøm, S.: Dayside magnetic ULF power at high latitudes: A possible long-term proxy for the solar wind velocity?, J. Geophys. Res.-Space, 104, 10145–10157, https://doi.org/10.1029/1999ja900015, 1999. a
Øieroset, M., Sandholt, P. E., Lühr, H., Denig, W. F., and Moretto, T.: Auroral and geomagnetic events at cusp/mantle latitudes in the prenoon sector during positive IMF By conditions: Signatures of pulsed magnetopause reconnection, J. Geophys. Res.-Space, 102, 7191–7205, https://doi.org/10.1029/96ja03716, 1997. a
Short summary
Rapid geomagnetic variations in the ultra-low frequency band are observed using ground-based magnetometers. We apply four years of data from West Greenland in a statistical analysis of the distribution of such variations. We identify a rapid geomagnetic variation population associated with the magnetospheric cusp that is separate from the auroral oval during summer. Earlier studies, which were mainly performed in winter, failed to unambiguously identify these variations.
Rapid geomagnetic variations in the ultra-low frequency band are observed using ground-based...