{"title":"Study of the thermospheric-ionospheric response to intense geomagnetic storms at middle latitudes","authors":"A. Belehaki , I. Tsagouri","doi":"10.1016/S1464-1917(01)00012-5","DOIUrl":"10.1016/S1464-1917(01)00012-5","url":null,"abstract":"<div><p>The ionospheric response to enhanced geomagnetic activity was studied in terms of two ionospheric parameters, f<sub>o</sub>F2 and h'F2, aiming the investigation of the middle latitude positive and negative ionospheric storm effects characteristics. Simultaneous observations from a chain of several middle latitude stations distributed in longitude around the earth during two intense geomagnetic storms (Dst < −100 nT), were analyzed in this work. The correlation results between the f<sub>o</sub>F2 and h'F2 disturbances and the Dst geomagnetic index verified that the morphology of middle latitude ionospheric disturbances in response to geomagnetic storms shows a great degree of variability and a strong dependence on local time observation. Negative deviations constitute the typical ionospheric response. In general it is reported that the F2 layer virtual height h'F2, which is observed only during daytime in conjunction with F1 layer presence, shows clear response to magnetic storm activity. On the other hand, positive ionospheric disturbances are accompanied by weak height enhancements. Real observations were also compared to the thermospheric-ionospheric view associated with positive and negative storm effects proposed by Prolss (1993). This test clearly demonstrates that such a model can capture most of the basic aspects of ionospheric storms, taking into consideration that any new burst of activity is associated to a new disturbance zone, resulting to the formation of a large zone of disturbance that covers the post-midnight and the forenoon sector as well. This mechanism may be the cause of long lasting negative storm effects observed as the typical ionospheric response to geomagnetic storm activity.</p></div>","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 5","pages":"Pages 353-357"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00012-5","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"87042426","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Observations of gravity waves of meteorological origin in the F-Region ionosphere","authors":"J. Boška, P. Šauli","doi":"10.1016/S1464-1917(01)00024-1","DOIUrl":"https://doi.org/10.1016/S1464-1917(01)00024-1","url":null,"abstract":"","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 6","pages":"425-428"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00024-1","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72293018","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
K.P. Nielsen , C.S. Deehr , E. Raustein , Y. Gjessing , F Sigernes
{"title":"Polar OH-airglow temperature variations in the 87/88 winter","authors":"K.P. Nielsen , C.S. Deehr , E. Raustein , Y. Gjessing , F Sigernes","doi":"10.1016/S1464-1917(01)00021-6","DOIUrl":"https://doi.org/10.1016/S1464-1917(01)00021-6","url":null,"abstract":"","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 6","pages":"405-410"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00021-6","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72243039","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Acoustic and ionospheric disturbances from point acoustic source","authors":"Ya.V. Drobheza , V.M. Krasnov","doi":"10.1016/S1464-1917(01)00027-7","DOIUrl":"https://doi.org/10.1016/S1464-1917(01)00027-7","url":null,"abstract":"","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 6","pages":"439-443"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00027-7","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72243041","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"VLF monitorig of atmosphere-ionosphere boundary as a tool to study planetary waves evolution and seismic influence","authors":"O.A. Molchanov , M. Hayakawa","doi":"10.1016/S1464-1917(01)00030-7","DOIUrl":"https://doi.org/10.1016/S1464-1917(01)00030-7","url":null,"abstract":"","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 6","pages":"453-458"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00030-7","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72243048","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Significance of water complexes in the atmosphere","authors":"J.E. Headrick, V. Vaida","doi":"10.1016/S1464-1917(01)00035-6","DOIUrl":"10.1016/S1464-1917(01)00035-6","url":null,"abstract":"<div><p>Using standard statistical and thermodynamic procedures, we calculate equilibrium constants for the formation of select, hydrogen-bonded water complexes, namely the water dimer and the cyclic trimer and tetramer, and use them to estimate the atmospheric abundances of these species. We generate water complex altitude profiles (0–30 km) for both a saturated and an unsaturated atmosphere and discuss the dominant factors influencing our results. In our analysis, particular emphasis is given to the significance that water monomer concentrations, complex binding energies, hydrogen-bond energies, and entropy have on the calculated abundance profiles. We examine the importance of enthalpy and entropy at atmospheric temperatures and show how each contributes to our calculated equilibrium constants. By applying a universal 2 °C temperature increase throughout the troposphere and lower stratosphere, we are able to model the effect that global warming would have on (H<sub>2</sub>O)<sub>n</sub> abundances in a saturated atmosphere. We also illustrate the effect that this thermal variation would have on entropy, enthalpy, and K<sub>p</sub>(T) values. Based on our results, we assess the atmospheric significance of water dimers and cyclic water complexes.</p></div>","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 7","pages":"Pages 479-486"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00035-6","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"81981944","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"The collision meter: An experimental technique to measure charged-neutral interactions and gas composition in the upper atmosphere","authors":"J.H. Clemmons , R.F. Pfaff","doi":"10.1016/S1464-1917(00)00116-1","DOIUrl":"10.1016/S1464-1917(00)00116-1","url":null,"abstract":"<div><p>A method of exploring the upper atmosphere through measurements of charged-neutral particle collisions is described. The method utilizes a charged particle beam which is injected into space from an in-situ probe and returns to the probe under its gyromotion about the ambient magnetic field. Measurements of the attenuation of the returned beam provide direct information on the collisional cross sections between the beam particles and the ambient medium. The method is discussed and expected measurements displayed and evaluated. In addition to providing new information on collision processes in the upper atmosphere, it is shown that this method has the potential for returning very accurate determinations of the densities of the major neutral gas species, including atomic oxygen. Initial in-situ experiments and directions for extension and further use are discussed.</p></div>","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 4","pages":"Pages 247-252"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(00)00116-1","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"80892498","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Two-dimensional simulation of two viscous debris flows in Austria","authors":"J. Hübl, H. Steinwendtner","doi":"10.1016/S1464-1917(01)00061-7","DOIUrl":"10.1016/S1464-1917(01)00061-7","url":null,"abstract":"<div><p>Risk mitigation and hazard assessment in steep torrent catchments requires a high level of information about possible runout distances, depth, velocities and resulting impact forces of mass movement processes and its consequences to endangered areas. Two well documented debris flow events at Wartschenbach/Eastern Tyrol and Moschergraben/Styria enable to investigate possible applications of the FLO-2D computer model. The FLO-2D computer model was developed at the Colorado State University and is a grid-based physical process model which routes precipitation-runoff and flood hydrographs over unconfined surfaces and channels using either a kinematic, diffusive or dynamic wave approximation to the momentum equation. All transitions between water floods and fully developed debris flows can be simulated using topographic data files to build the grid elements, information about surface roughness and properties of the sediment water mixture. A quadratic rheological model is used to describe flow behaviour of viscous debris flows. The rheological properties of deposited debris flow material are determined using a rotational viscometer and a new developed conveyor-channel.</p><p>The simulation results and the gained experience are of great promise to the future of debris flow modelling.</p></div>","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 9","pages":"Pages 639-644"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00061-7","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"78345721","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
{"title":"Auroral particle acceleration processes: the legacy of Hannes Alfvén","authors":"R. Lundin","doi":"10.1016/S1464-1917(00)00085-4","DOIUrl":"https://doi.org/10.1016/S1464-1917(00)00085-4","url":null,"abstract":"<div><p>Impacting corpuscular radiation was believed to be the main cause for the aurora even before the space age. However, the means by which charged particles become energized, eventually impacting into the upper atmosphere was a matter of controversy - a controversy which died out only very slowly with time. Hannes Alfvén was the lead scientists in the 1950:ies and 1960:ies who dared to challenge the ruling paradigm of space plasma physics - by 1958 suggesting field-aligned electric “discharges” as the cause of the aurora. Field-aligned electric acceleration of charged particles became a matter of debate for nearly three decades with indirect proofs for its existence steadily mounting with time, yet all the time meeting strong objections. In retrospect one may wonder why rebutting was so important. Why clinging to the concept of infinite conductivity along magnetic field lines? The reason was simple, because it challenged a ruling paradigm in space plasma physics, requiring a strong modification of “ideal MHD”.</p><p>The notion of “frozen-in-field-lines”, invented by Hannes Alfvén, is a useful concept in describing large scale morphologies. However, observations from space plasma experiments shows that the condition of frozen-in-field-lines is violated in most interesting regions where plasma acceleration occurs. Alfvén wanted to remedy what he considered the “misuse of MHD” by emphasizing currents instead of magnetic fields in space plasma physics.</p><p>In this paper I will review the energy and momentum coupling originally proposed by Alfvén and their consequences for the acceleration of charged particles. Plasma acceleration processes, well known and recognized from studies of planetary magnetospheres in our solar system, are applicable also for more remote space objects in the Universe - such as stars and galaxies. The many astrophysical implications of his theories is perhaps the most important legacy of Hannes Alfvén. In fact, new evidence for his theories are emerging from contemporary deep space data.</p></div>","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 1","pages":"Pages 13-23"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(00)00085-4","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"91669475","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
C. Cattell , J. Dombeck , A. Keiling , J. Wygant , R. Bergmann , M.K. Hudson , C. Kletzing , F.S. Mozer , M. Temerin , I. Roth , G. Parks
{"title":"Comparison of solitary waves and wave packets observed at plasma sheet boundary to results from the auroral zone","authors":"C. Cattell , J. Dombeck , A. Keiling , J. Wygant , R. Bergmann , M.K. Hudson , C. Kletzing , F.S. Mozer , M. Temerin , I. Roth , G. Parks","doi":"10.1016/S1464-1917(00)00095-7","DOIUrl":"https://doi.org/10.1016/S1464-1917(00)00095-7","url":null,"abstract":"<div><p>The plasma sheet boundary, at distances intermediate between the auroral acceleration region and the regions where energy conversion associated with substorms occurs, is very dynamic with electron and ion beams, field-aligned currents and many types of waves and non-linear structures. We discuss electric and magnetic fields observations of waves occurring at two very different time-scales. At the longer scales (10's of seconds), Wygant (2000) have shown that the observed fields are associated with Alfvenic fluctuations which have their largest electric field normal to the average plane of the plasma sheet (δE<sub>N</sub>). The simultaneously observed magnetic field perturbations are azimuthal(δB<sub>T</sub>), resulting in a Poynting flux along the geomagnetic field. The observations are consistent with an incompressible, transverse electromagnetic surface shear Alfven mode at the surface of the plasma sheet boundary. The local δE<sub>N</sub>/δB<sub>T</sub> is consistent with V<sub>A</sub>. The waves provide an intense earthward Poynting flux sufficient to provide the energy necessary for the energization of auroral electron beams. In addition, the large amplitude surface waves are magnetically conjugate (to within 1 degree) to intense auroral emission as determined from the UVI imager, whereas weak aurora are correlated with small amplitude electric fields. Particle detectors simultaneously observe ions flowing up the field line away from the earth, providing further evidence that low altitude acceleration is occurring on conjugate magnetic field lines. At small scales, large amplitude solitary waves are frequently observed, and ion acoustic, lower hybrid, and Langmuir wave packets are sometimes seen. There are clear differences between the solitary wave observations at the plasma sheet boundary and in the low altitude auroral zone. At high altitudes, only electron mode solitary waves have been identified and they occur both in regions of upward and downward field-aligned current, in contrast to the auroral zone where ion solitary waves occur in upward currents and electron solitary waves occur primarily in downward currents. This difference may because the growth of ion acoustic solitons requires that the plasma be strongly magnetized (f<sub>ce</sub>/f<sub>pe</sub> >>1) which is not the case for the observed high altitude plasma sheet boundary crossings. The high altitude events are associated with a wide variety of electron distribution types, whereas the low altitude events occur in regions of flat-top electron beam distributions. Preliminary evidence suggests that the high altitude events may be BGK electron holes, as has been shown for the low altitude events. For the parameter regime usually observed at high attitudes, electron holes would be stable. In addition, initial work on electron acoustic solitons suggests that these compressive waves would occur only for a limited range of parameters, so they are unlikely to explain t","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 1","pages":"Pages 97-106"},"PeriodicalIF":0.0,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(00)00095-7","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"91669911","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}