Investigating Plasma Storms and Substorms in Our Near-Earth Backyard
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A Nonstorm Time Enhancement of Relativistic Electrons in the Outer Radiation Belt Quintin Schiller,1,2 Xinlin Li,1,2 Lauren Blum,1,2 Weichao Tu,3 Drew L
GEOPHYSICAL RESEARCH LETTERS, VOL. 41, 7–12, doi:10.1002/2013GL058485, 2014 A nonstorm time enhancement of relativistic electrons in the outer radiation belt Quintin Schiller,1,2 Xinlin Li,1,2 Lauren Blum,1,2 Weichao Tu,3 Drew L. Turner,4 and J. B. Blake5 Received 29 October 2013; revised 27 November 2013; accepted 28 November 2013; published 15 January 2014. [1] Despite the lack of a geomagnetic storm (based on the [3] Acceleration mechanisms, which replenish the relativ- Dst index), relativistic electron fluxes were enhanced over istic electron content, can be classified into two broad catego- 2.5 orders of magnitude in the outer radiation belt in 13 h ries: radial transport and internal acceleration. Radial on 13–14 January 2013. The unusual enhancement was transport mechanisms can again be broadly classified into observed by Magnetic Electron Ion Spectrometer (MagEIS), two subcategories: radial diffusion and sudden injection, onboard the Van Allen Probes; Relativistic Electron and both of which violate the third adiabatic invariant. Radial Proton Telescope Integrated Little Experiment, onboard transport requires an electron source population at high L, the Colorado Student Space Weather Experiment; and such as the plasma sheet in the tail of the magnetosphere Solid State Telescope, onboard Time History of Events [e.g., Ingraham et al., 2001]. Radial transport by diffusion and Macroscale Interactions during Substorms (THEMIS). in the third adiabatic invariant is a result of incoherent scatter- Analyses of MagEIS phase space density (PSD) profiles ing by ULF waves in the Pc4–5 band [e.g., Tu et al., 2012]. show a positive outward radial gradient from 4 < L < 5.5. -
Analysis of Geomagnetic Storms in South Atlantic Magnetic Anomaly (SAMA)
Analysis of geomagnetic storms in South Atlantic Magnetic Anomaly (SAMA) Júlia Maria Soja Sampaio, Elder Yokoyama, Luciana Figueiredo Prado Copyright 2019, SBGf - Sociedade Brasileira de Geofísica Moreover, Dst and AE indices may vary according to the This paper was prepared for presentation during the 16th International Congress of the geomagnetic field geometry, such as polar to intermediate Brazilian Geophysical Society held in Rio de Janeiro, Brazil, 19-22 August 2019. latitudinal field variations. In this framework, fluctuations Contents of this paper were reviewed by the Technical Committee of the 16th in the geomagnetic field can occur under the influence of International Congress of the Brazilian Geophysical Society and do not necessarily represent any position of the SBGf, its officers or members. Electronic reproduction or the South Atlantic Magnetic Anomaly (SAMA). The SAMA storage of any part of this paper for commercial purposes without the written consent is a region of minimum geomagnetic field intensity values of the Brazilian Geophysical Society is prohibited. ____________________________________________________________________ at the Earth’s surface (Figure 1), and its dipole intensity is decreasing along the past 1000 years (Terra-Nova et. al., Abstract 2017). Geomagnetic storm is a major disturbance of Earth’s In this study we will compare the behavior of the types of magnetosphere resulted from the interaction of solar wind geomagnetic storms basis on AE and Dst indices. and the Earth’s magnetic field. This disturbance depends of the Earth magnetic field geometry, and varies in terms of intensity from the Poles to the Equator. This disturbance is quantified through geomagnetic indices, such as the Dst and the AE indices. -
Information Summaries
TIROS 8 12/21/63 Delta-22 TIROS-H (A-53) 17B S National Aeronautics and TIROS 9 1/22/65 Delta-28 TIROS-I (A-54) 17A S Space Administration TIROS Operational 2TIROS 10 7/1/65 Delta-32 OT-1 17B S John F. Kennedy Space Center 2ESSA 1 2/3/66 Delta-36 OT-3 (TOS) 17A S Information Summaries 2 2 ESSA 2 2/28/66 Delta-37 OT-2 (TOS) 17B S 2ESSA 3 10/2/66 2Delta-41 TOS-A 1SLC-2E S PMS 031 (KSC) OSO (Orbiting Solar Observatories) Lunar and Planetary 2ESSA 4 1/26/67 2Delta-45 TOS-B 1SLC-2E S June 1999 OSO 1 3/7/62 Delta-8 OSO-A (S-16) 17A S 2ESSA 5 4/20/67 2Delta-48 TOS-C 1SLC-2E S OSO 2 2/3/65 Delta-29 OSO-B2 (S-17) 17B S Mission Launch Launch Payload Launch 2ESSA 6 11/10/67 2Delta-54 TOS-D 1SLC-2E S OSO 8/25/65 Delta-33 OSO-C 17B U Name Date Vehicle Code Pad Results 2ESSA 7 8/16/68 2Delta-58 TOS-E 1SLC-2E S OSO 3 3/8/67 Delta-46 OSO-E1 17A S 2ESSA 8 12/15/68 2Delta-62 TOS-F 1SLC-2E S OSO 4 10/18/67 Delta-53 OSO-D 17B S PIONEER (Lunar) 2ESSA 9 2/26/69 2Delta-67 TOS-G 17B S OSO 5 1/22/69 Delta-64 OSO-F 17B S Pioneer 1 10/11/58 Thor-Able-1 –– 17A U Major NASA 2 1 OSO 6/PAC 8/9/69 Delta-72 OSO-G/PAC 17A S Pioneer 2 11/8/58 Thor-Able-2 –– 17A U IMPROVED TIROS OPERATIONAL 2 1 OSO 7/TETR 3 9/29/71 Delta-85 OSO-H/TETR-D 17A S Pioneer 3 12/6/58 Juno II AM-11 –– 5 U 3ITOS 1/OSCAR 5 1/23/70 2Delta-76 1TIROS-M/OSCAR 1SLC-2W S 2 OSO 8 6/21/75 Delta-112 OSO-1 17B S Pioneer 4 3/3/59 Juno II AM-14 –– 5 S 3NOAA 1 12/11/70 2Delta-81 ITOS-A 1SLC-2W S Launches Pioneer 11/26/59 Atlas-Able-1 –– 14 U 3ITOS 10/21/71 2Delta-86 ITOS-B 1SLC-2E U OGO (Orbiting Geophysical -
Emission of Cosmic Rays from Jupiter. Magnetospheres As Possible Sources of Cosmic Rays
EPJ manuscript No. (will be inserted by the editor) Emission of cosmic rays from Jupiter. Magnetospheres as possible Sources of Cosmic Rays G.Pizzella Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati Received: date / Revised version: date Abstract. Measurements made recently with the PAMELA satellite have shown with good evidence that a fraction of the cosmic rays detected on Earth comes from Jupiter. This result draws attention to the idea that magnetospheres of astrophysical objects could contribute to the sources of cosmic rays. We discuss this conjecture on the basis of Earth installed instrumentation and of the measurements made with PAMELA. The experiments strongly favor the validity of the conjecture. In particular the PAMELA data show that the proton fluxes are larger when the Earth orbit intersects the lines of the interplanetary magnetic field connecting Jupiter with Earth. This effect shows up with more than ten standard deviations, difficult to explain without the idea that part of the cosmic ray protons comes directly from the Jupiter magnetosphere. PACS. 94.30 Magnetosphere { 98.40.S Cosmic Rays 1 Introduction 2 The trapped radiation An unexpected discovery was the Van Allen belt in 1958. It has been recently published a paper [1] showing good Although in earlier times Kristian Birkeland, Carl St¨ormer, evidence that a small but not negligible fraction of cos- and Nicholas Christofilos considered the possibility that mic rays detected by the Earth satellite PAMELA1 comes fluxes of charged particles could dwell in the magnetic field from the planet Jupiter. The suggestion was that higher surrounding the Earth, nobody was expecting so large energy particles leak out from the Jupiter trapped particle density of charged particle population that formed a sort region and then are ejected into space following the inter- of permanent belt surrounding the Earth. -
On Magnetic Storms and Substorms
ILWS WORKSHOP 2006, GOA, FEBRUARY 19-24, 2006 On magnetic storms and substorms G. S. Lakhina, S. Alex, S. Mukherjee and G. Vichare Indian Institute of Geomagnetism, New Panvel (W), Navi Mumbai-410218, India Abstract. Magnetospheric substorms and storms are indicators of geomagnetic activity. Whereas the geomagnetic index AE (auroral electrojet) is used to study substorms, it is common to characterize the magnetic storms by the Dst (disturbance storm time) index of geomagnetic activity. This talk discusses briefly the storm-substorms relationship, and highlights some of the characteristics of intense magnetic storms, including the events of 29-31 October and 20-21 November 2003. The adverse effects of these intense geomagnetic storms on telecommunication, navigation, and on spacecraft functioning will be discussed. Index Terms. Geomagnetic activity, geomagnetic storms, space weather, substorms. _____________________________________________________________________________________________________ 1. Introduction latitude magnetic fields are significantly depressed over a Magnetospheric storms and substorms are indicators of time span of one to a few hours followed by its recovery geomagnetic activity. Where as the magnetic storms are which may extend over several days (Rostoker, 1997). driven directly by solar drivers like Coronal mass ejections, solar flares, fast streams etc., the substorms, in simplest terms, are the disturbances occurring within the magnetosphere that are ultimately caused by the solar wind. The magnetic storms are characterized by the Dst (disturbance storm time) index of geomagnetic activity. The substorms, on the other hand, are characterized by geomagnetic AE (auroral electrojet) index. Magnetic reconnection plays an important role in energy transfer from solar wind to the magnetosphere. Magnetic reconnection is very effective when the interplanetary magnetic field is directed southwards leading to strong plasma injection from the tail towards the inner magnetosphere causing intense auroras at high-latitude nightside regions. -
The Need for Detailed Ionic Composition of the Near-Earth Plasma
HeliophysicsHELIO 2050 2050 White Papers (2021) R. Ilie4094.pdf THE NEED FOR DETAILED IONIC COMPOSITION OF THE NEAR-EARTH PLASMA An impressive body of work has been devoted to the escape of H+, He+ and O+ ions from Earth’s ionosphere, and their circulation and redistribution throughout the terrestrial magneto- sphere (Schunk and Raitt, 1980; Schunk and Sojka, 1997; Winglee et al., 2002; Glocer et al., 2009; Ilie et al., 2015; Ilie and Liemohn, 2016). However, the transport and energization of N+, in addi- tion to that of O+, has not been considered by most studies, even though a number of direct and indirect measurements made to describe the ionic composition of the ionosphere-magnetosphere system, have established that N+ is a significant ion species in the ionosphere and its presence in the magnetosphere is significant. A wide range in the magnitude oftheN+ to O+ density ratio has been reported, with significant variations not only with geomagnetic activity, but also with solar cycle, season, time of day, latitude, etc (Mall et al., 2002; Christon et al., 2002). These vari- ations suggest that N+ and O+, while relatively close in mass, they obey different chemical and energization processes, and possibly follow different paths of energization. In addition, observations from the WIND STICS ISIS 2 spacecraft (Hoffman et al., 1974) indicated that not only N+, but also molecular ions were ob- served in the Earth’s magnetosphere Geotail STICS AMPTE and ionosphere. Measurements from CCE Explorer 31 Akebono SMS the Arase satellite (Miyoshi et al., MMS ISIS-2 IMS DE-1 RIMSS e-POP 2018) showed the existence of molec- OGO-6 OGOGO-2-2 IMSS Sputnik3 IMS AE-C ular ions in the Earth’s ring cur- RMS IMS rent region, even under moderate ge- omagnetic storm conditions. -
Planetary Magnetospheres
CLBE001-ESS2E November 9, 2006 17:4 100-C 25-C 50-C 75-C C+M 50-C+M C+Y 50-C+Y M+Y 50-M+Y 100-M 25-M 50-M 75-M 100-Y 25-Y 50-Y 75-Y 100-K 25-K 25-19-19 50-K 50-40-40 75-K 75-64-64 Planetary Magnetospheres Margaret Galland Kivelson University of California Los Angeles, California Fran Bagenal University of Colorado, Boulder Boulder, Colorado CHAPTER 28 1. What is a Magnetosphere? 5. Dynamics 2. Types of Magnetospheres 6. Interaction with Moons 3. Planetary Magnetic Fields 7. Conclusions 4. Magnetospheric Plasmas 1. What is a Magnetosphere? planet’s magnetic field. Moreover, unmagnetized planets in the flowing solar wind carve out cavities whose properties The term magnetosphere was coined by T. Gold in 1959 are sufficiently similar to those of true magnetospheres to al- to describe the region above the ionosphere in which the low us to include them in this discussion. Moons embedded magnetic field of the Earth controls the motions of charged in the flowing plasma of a planetary magnetosphere create particles. The magnetic field traps low-energy plasma and interaction regions resembling those that surround unmag- forms the Van Allen belts, torus-shaped regions in which netized planets. If a moon is sufficiently strongly magne- high-energy ions and electrons (tens of keV and higher) tized, it may carve out a true magnetosphere completely drift around the Earth. The control of charged particles by contained within the magnetosphere of the planet. -
IONIZING RADIATION EXPOSURE Grade Level 11–12
IONIZING RADIATION EXPOSURE Grade Level 11–12 Instructional Objectives Key Topic Students will Atomic physics • practice and review atomic physics concepts and equations; Degree of Difficulty • apply Planck’s constant; Moderate • determine the deBroglie wavelength of a proton; and analyze the frequency of photons. • Teacher Prep Time 10 minutes Degree of Difficulty For the average student in AP Physics B, this problem is moderately difficult Class Time Required due to the limited amount of time available in AP Physics B to the study of 25–35 minutes atomic and nuclear physics. Students should be provided with the mass of a proton, speed of light, and the necessary equations located on the AP Technology physics equation sheet. - TI-Nspire™ Learning Handhelds For part C, students should understand the relationship between frequency - TI-Nspire document: and energy of electromagnetic waves, and the relationship between the Ionizing_Radiation.tns speed of these waves, both in wavelength and frequency. Materials Class Time Required AP Physics equation sheet This problem requires 25–35 minutes. -------------------------------- • Introduction: 10 minutes o Read and discuss the background section with the class before Learning Objectives for students work on the problem. AP Physics Atomic and Nuclear Student Work Time: 10–15 minutes • Physics: • Post Discussion: 5–10 minutes - Atomic Physics and Quantum Effects Background NSES This problem is part of a series of problems that apply Math and Science Standards Science @ Work in NASA’s research facilities. - Physical Science The International Space Station (ISS) orbits the Earth at an approximate - Science in Personal and altitude of 407 km (252 mi). At this altitude, astronauts are not as well Social Perspectives protected by the Earth’s atmosphere, and are exposed to higher levels of - History and Nature of space radiation than what is experienced on the Earth’s surface. -
Acceleration of Particles to High Energies in Earth's Radiation Belts
Space Sci Rev (2012) 173:103–131 DOI 10.1007/s11214-012-9941-x Acceleration of Particles to High Energies in Earth’s Radiation Belts R.M. Millan · D.N. Baker Received: 16 April 2012 / Accepted: 30 September 2012 / Published online: 25 October 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract Discovered in 1958, Earth’s radiation belts persist in being mysterious and un- predictable. This highly dynamic region of near-Earth space provides an important natural laboratory for studying the physics of particle acceleration. Despite the proximity of the ra- diation belts to Earth, many questions remain about the mechanisms responsible for rapidly energizing particles to relativistic energies there. The importance of understanding the ra- diation belts continues to grow as society becomes increasingly dependent on spacecraft for navigation, weather forecasting, and more. We review the historical underpinning and observational basis for our current understanding of particle acceleration in the radiation belts. Keywords Particle acceleration · Radiation belts · Magnetosphere 1 Introduction 1.1 Motivation Shortly after the discovery of Earth’s radiation belts, the suggestion was put forward that processes occurring locally, in near-Earth space, might be responsible for the high energy particles observed there. Efforts were also carried out to search for an external source that could inject multi-MeV electrons into Earth’s inner magnetosphere where they could then be trapped by the magnetic field. Energetic electrons are in fact observed in interplanetary space, originating at both Jupiter and the sun. However, the electron intensity in Earth’s radiation belts is not correlated with the interplanetary intensity, and a significant external R.M. -