aariПроблемы Арктики и АнтарктикиArctic and Antarctic Research0555-26482618-6713Государственный научный центр Российской Федерации Арктический и антарктический научно-исследовательский институт10.30758/0555-2648-2018-64-2-141-156aari-11Research ArticleФИЗИКА АТМОСФЕРЫ И ГИДРОСФЕРЫATMOSPHERE AND HYDROSPHERE PHYSICSПолярные сияния в каспе и его приполюсной окрестности: исследование отдельного событияAuroras in the cusp and its poleward vicinity: a case studyСафаргалеевВ. В.SafargaleevV. V.

Apatity

vladimir.safargaleev@pgia.ruСергиенкоТ. И.SergienkoT. I.

Кируна

Kirun

Полярный геофизический институт РАНРоссияPolar Geophysical Institute RASRussian FederationШведский институт космической физикиШвецияSwedish Institute of Space PhysicsSweden201830062018642141156Copyright © Сафаргалеев В.В., Сергиенко Т.И., 20182018Сафаргалеев В.В., Сергиенко Т.И.Safargaleev V.V., Sergienko T.I.Данная работа распространяется под лицензией Creative Commons Attribution 4.0.This work is licensed under a Creative Commons Attribution 4.0 License.https://www.aaresearch.science/jour/article/view/11

Исследован редкий случай одновременной регистрации дневных полярных сияний наземной оптической аппаратурой и детектором высыпающихся частиц на спутниках DMSP F16 и F17. Оптические измерения проводились камерой полного обзора неба Полярного геофизического института, установленной в обсерватории Баренцбург на арх. Шпицберген. Следуя развороту вертикальной компоненты межпланетного магнитного поля (Bz-компоненты ММП) в область отрицательных значений, система слабых лучистых дуг сместилась к югу, после чего одна из дуг начала дрейфовать обратно к полюсу и пропала. Спутник DMSP F17 пересек касп спустя двадцать минут после разворота Bz-компоненты. Совместный анализ оптических и спутниковых данных показал, что наблюдаемые слабые лучистые структуры находятся в области каспенных высыпаний и пространственно связаны с всплеском высыпающихся электронов с энергией менее 100 эВ. Следующий спутник DMSP пересек поле  зрения камеры спустя десять минут после первого,  и анализ его данных показал, что эта дуга в момент исчезновения находилась в области разомкнутых силовых линий. Этот результат, дополненный специфической формой протонных высыпаний в данных спутника DMSP, которую традиционно связывают с пересоединением, позволил нам прийти к выводу, что смещавшаяся к полюсу слабая лучистая дуга могла представлять собой ионосферный след только что пересоединившейся магнитной силовой трубки, уносимой солнечным ветром в антисолнечном направлении. Оценена высота и поперечный размер элемента лучистой структуры в каспе.

Summary We present a case study of the dayside aurora observed simultaneously with optical instruments from the ground and with auroral particle spectrometers aboard the DMSP F16 and F17 satellites. Optical observations were carried out with an all-sky camera at the Polar Geophysical Institute (PGI) observatory Barentsburg on Svalbard. The aurora as a whole moved equatorward in response to negative turning of the IMF Bz component and then the distinct faint rayed arc intensified, moved to the north and faded. Satellite DMSP F17 crossed the cusp twenty minutes after Bz turned southward. Joint analysis of optical and satellite data showed that faint auroral structures are embedded into the cusp precipitations and correspond to the bursts of electron precipitations with energy below 100 eV. The next satellite crossed the camera field-of-view ten minutes later and the data showed that the source of the faded poleward moving rayed arc was located, most probably, on the non-closed magnetic field lines. This finding and the presence of ion-energy dispersion in the DMSP data allows us to make the conclusion that the dayside reconnection may be considered as the reason for this kind of aurora activity. In this study we also estimated the altitude and horizontal scale of auroral rays in the cusp.

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The authors declare that there are no conflicts of interest present.