Probabilistic seismic source inversion from regional landslide evidence     

Rasanen  Ryan A.  Maurer  Brett W. 《Landslides》2022,19(2):407-419

Landslides - In regions of infrequent but potentially damaging seismicity, modern earthquake inventories may be insufficient to provide inputs to seismic hazard analyses (i.e., fault locations and...  相似文献   

Rethinking big data in digital humanitarianism: practices,epistemologies, and social relations   总被引：1，自引：0，他引：1  

Ryan Burns 《GeoJournal》2015,80(4):477-490

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The history of subaquatic volcanism recorded in the sediments of Lake Kivu; East Africa     

Kelly Ann Ross  Martin Schmid  Sandra Ogorka  Fabrice A. Muvundja  Flavio S. Anselmetti 《Journal of Paleolimnology》2015,54(1):137-152

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Quantified,multi-scale X-ray fluorescence element mapping using the Maia detector array: application to mineral deposit studies     

Louise A. Fisher  Denis Fougerouse  James S. Cleverley  Christopher G. Ryan  Steven Micklethwaite  Angela Halfpenny  Robert M. Hough  Mary Gee  David Paterson  Daryl L. Howard  Kathryn Spiers 《Mineralium Deposita》2015,50(6):665-674

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Extreme Ultra-Violet Spectroscopy of the Lower Solar Atmosphere During Solar Flares (Invited Review)     

Ryan O. Milligan 《Solar physics》2015,290(12):3399-3423

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Benchmark Test of Differential Emission Measure Codes and Multi-thermal Energies in Solar Active Regions     

Markus J. Aschwanden  Paul Boerner  Amir Caspi  James M. McTiernan  Daniel Ryan  Harry Warren 《Solar physics》2015,290(10):2733-2763

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Exoplanet atmospheres with EChO: spectral retrievals using EChOSim     

Joanna K. Barstow  Neil E. Bowles  Suzanne Aigrain  Leigh N. Fletcher  Patrick G. J. Irwin  Ryan Varley  Enzo Pascale 《Experimental Astronomy》2015,40(2-3):545-561

We demonstrate the effectiveness of the Exoplanet Characterisation Observatory mission concept for constraining the atmospheric properties of hot and warm gas giants and super Earths. Synthetic primary and secondary transit spectra for a range of planets are passed through EChOSim [13] to obtain the expected level of noise for different observational scenarios; these are then used as inputs for the NEMESIS atmospheric retrieval code and the retrieved atmospheric properties (temperature structure, composition and cloud properties) compared with the known input values, following the method of [1]. To correctly retrieve the temperature structure and composition of the atmosphere to within 2 σ, we find that we require: a single transit or eclipse of a hot Jupiter orbiting a sun-like (G2) star at 35 pc to constrain the terminator and dayside atmospheres; 20 transits or eclipses of a warm Jupiter orbiting a similar star; 10 transits/eclipses of a hot Neptune orbiting an M dwarf at 6 pc; and 30 transits or eclipses of a GJ1214b-like planet.  相似文献   

The Compatibility of Flare Temperatures Observed with AIA,GOES, and RHESSI     

Daniel F. Ryan  Aidan M. O’Flannagain  Markus J. Aschwanden  Peter T. Gallagher 《Solar physics》2014,289(7):2547-2563

We test the compatibility and biases of multi-thermal flare DEM (differential emission measure) peak temperatures determined with AIA with those determined by GOES and RHESSI using the isothermal assumption. In a set of 149 M- and X-class flares observed during the first two years of the SDO mission, AIA finds DEM peak temperatures at the time of the peak GOES 1?–?8 Å flux to have an average of T _p=12.0±2.9 MK and Gaussian DEM widths of log₁₀(σ _T )=0.50±0.13. From GOES observations of the same 149 events, a mean temperature of T _p=15.6±2.4 MK is inferred, which is systematically higher by a factor of T _GOES/T _AIA=1.4±0.4. We demonstrate that this discrepancy results from the isothermal assumption in the inversion of the GOES filter ratio. From isothermal fits to photon spectra at energies of ?≈6?–?12 keV of 61 of these events, RHESSI finds the temperature to be higher still by a factor of T _RHESSI/T _AIA=1.9±1.0. We find that this is partly a consequence of the isothermal assumption. However, RHESSI is not sensitive to the low-temperature range of the DEM peak, and thus RHESSI samples only the high-temperature tail of the DEM function. This can also contribute to the discrepancy between AIA and RHESSI temperatures. The higher flare temperatures found by GOES and RHESSI imply correspondingly lower emission measures. We conclude that self-consistent flare DEM temperatures and emission measures require simultaneous fitting of EUV (AIA) and soft X-ray (GOES and RHESSI) fluxes.  相似文献   

Sutter's Mill dicarboxylic acids as possible tracers of parent‐body alteration processes     

Sandra Pizzarello  Laurence A. J. Garvie 《Meteoritics & planetary science》2014,49(11):2087-2094

Dicarboxylic acids were searched for in three Sutter's Mill (SM) fragments (SM2 collected prerain, SM12, and SM41) and found to occur almost exclusively as linear species of 3‐ to 14‐carbon long. Between these, concentrations were low, with measured quantities typically less than 10 nmole g^?1 of meteorite and a maximum of 6.8 nmole g^?1 of meteorite for suberic acid in SM12. The SM acids' molecular distribution is consistent with a nonbiological origin and differs from those of CMs, such as Murchison or Murray, and of some stones of the C2‐ungrouped Tagish Lake meteorite, where they are abundant and varied. Powder X‐ray diffraction of SM12 and SM41 show them to be dominated by clays/amorphous material, with lesser amounts of Fe‐sulfides, magnetite, and calcite. Thermal gravimetric (TG) analysis shows mass losses up to 1000 °C of 11.4% (SM12) and 9.4% (SM41). These losses are low compared with other clay‐rich carbonaceous chondrites, such as Murchison (14.5%) and Orgueil (21.1%). The TG data are indicative of partially dehydrated clays, in accordance with published work on SM2, for which mineralogical studies suggest asteroidal heating to around 500 °C. In view of these compositional traits and mineralogical features, it is suggested that the dicarboxylic acids observed in the SM fragments we analyzed likely represent a combination of molecular species original to the meteorite as well as secondary products formed during parent‐body alteration processes, such as asteroidal heating.  相似文献   

Frederick Drummond Gallie, 1912–1986     

Bruce Ryan 《The Australian geographer》1987,18(1)

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