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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2018
    In:  Journal of Geophysical Research: Space Physics Vol. 123, No. 2 ( 2018-02), p. 1279-1294
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 123, No. 2 ( 2018-02), p. 1279-1294
    Abstract: Case studies of relativistic microbursts with EMIC and/or chorus waves occurring are presented Statistically, there is an increase in VLF wave amplitude at the time of relativistic microbursts, consistent with chorus Statistically, there is no increase in EMIC activity at the time of relativistic microbursts
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    URL: Issue
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2018
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2019
    In:  Journal of Geophysical Research: Space Physics Vol. 124, No. 4 ( 2019-04), p. 2682-2696
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 124, No. 4 ( 2019-04), p. 2682-2696
    Abstract: Models accounting for transionospheric absorption and subionospheric attenuation improve satellite‐ground VLF PSD correlations Validation of these empirical models resulted in correlations between predicted and observed satellite VLF PSD of up to 0.764 Ground VLF receivers spaced around the Earth could provide longitudinal coverage of outer radiation belt chorus over ±45–75° latitude
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2019
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2018
    In:  Journal of Geophysical Research: Space Physics Vol. 123, No. 6 ( 2018-06), p. 4755-4766
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 123, No. 6 ( 2018-06), p. 4755-4766
    Abstract: Regression analyses of relativistic electron flux (0.7‐7.8 MeV) show both linear and nonlinear response to wave activity High chorus intensity and midrange ULF Pc5 power result in more electron acceleration than would be predicted by an additive model The negative effect of EMIC waves is greater if combined with either chorus or ULF Pc5 waves
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2018
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2015
    In:  Journal of Geophysical Research: Space Physics Vol. 120, No. 5 ( 2015-05), p. 3618-3631
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 120, No. 5 ( 2015-05), p. 3618-3631
    Abstract: EMIC induced electron precipitation with latitudinal width of 2–3° EMIC induced electron precipitation with lower cutoff energy of 280 keV Oxygen band EMIC induced electron precipitation driven by substorm
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    URL: Issue
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2015
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2016
    In:  Journal of Geophysical Research: Space Physics Vol. 121, No. 6 ( 2016-06), p. 5366-5383
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 121, No. 6 ( 2016-06), p. 5366-5383
    Abstract: POES‐based electron precipitation triggers most likely caused by EMIC waves detected on the ground EMIC‐IPDP repeatedly triggered at a single MLT closely tied to POES‐detected electron precipitation EMIC waves detected via POES‐detected electron precipitation are primarily helium band IPDP waves
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    URL: Issue
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2016
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 6
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2019
    In:  Journal of Geophysical Research: Space Physics Vol. 124, No. 5 ( 2019-05), p. 3729-3742
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 124, No. 5 ( 2019-05), p. 3729-3742
    Abstract: Subionospheric radio wave measurements show a sunrise transition during which a phase perturbation is often observed Sunrise phase perturbation amplitude is better correlated with stratospheric ozone number density than with atmospheric temperature Sunrise phase perturbation is principally generated by stratospheric ozone shadowing of the D region ionosphere
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2019
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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  • 7
    In: Geoscientific Model Development, Copernicus GmbH, Vol. 10, No. 6 ( 2017-06-22), p. 2247-2302
    Abstract: Abstract. This paper describes the recommended solar forcing dataset for CMIP6 and highlights changes with respect to CMIP5. The solar forcing is provided for radiative properties, namely total solar irradiance (TSI), solar spectral irradiance (SSI), and the F10.7 index as well as particle forcing, including geomagnetic indices Ap and Kp, and ionization rates to account for effects of solar protons, electrons, and galactic cosmic rays. This is the first time that a recommendation for solar-driven particle forcing has been provided for a CMIP exercise. The solar forcing datasets are provided at daily and monthly resolution separately for the CMIP6 preindustrial control, historical (1850–2014), and future (2015–2300) simulations. For the preindustrial control simulation, both constant and time-varying solar forcing components are provided, with the latter including variability on 11-year and shorter timescales but no long-term changes. For the future, we provide a realistic scenario of what solar behavior could be, as well as an additional extreme Maunder-minimum-like sensitivity scenario. This paper describes the forcing datasets and also provides detailed recommendations as to their implementation in current climate models.For the historical simulations, the TSI and SSI time series are defined as the average of two solar irradiance models that are adapted to CMIP6 needs: an empirical one (NRLTSI2–NRLSSI2) and a semi-empirical one (SATIRE). A new and lower TSI value is recommended: the contemporary solar-cycle average is now 1361.0 W m−2. The slight negative trend in TSI over the three most recent solar cycles in the CMIP6 dataset leads to only a small global radiative forcing of −0.04 W m−2. In the 200–400 nm wavelength range, which is important for ozone photochemistry, the CMIP6 solar forcing dataset shows a larger solar-cycle variability contribution to TSI than in CMIP5 (50 % compared to 35 %).We compare the climatic effects of the CMIP6 solar forcing dataset to its CMIP5 predecessor by using time-slice experiments of two chemistry–climate models and a reference radiative transfer model. The differences in the long-term mean SSI in the CMIP6 dataset, compared to CMIP5, impact on climatological stratospheric conditions (lower shortwave heating rates of −0.35 K day−1 at the stratopause), cooler stratospheric temperatures (−1.5 K in the upper stratosphere), lower ozone abundances in the lower stratosphere (−3 %), and higher ozone abundances (+1.5 % in the upper stratosphere and lower mesosphere). Between the maximum and minimum phases of the 11-year solar cycle, there is an increase in shortwave heating rates (+0.2 K day−1 at the stratopause), temperatures ( ∼  1 K at the stratopause), and ozone (+2.5 % in the upper stratosphere) in the tropical upper stratosphere using the CMIP6 forcing dataset. This solar-cycle response is slightly larger, but not statistically significantly different from that for the CMIP5 forcing dataset.CMIP6 models with a well-resolved shortwave radiation scheme are encouraged to prescribe SSI changes and include solar-induced stratospheric ozone variations, in order to better represent solar climate variability compared to models that only prescribe TSI and/or exclude the solar-ozone response. We show that monthly-mean solar-induced ozone variations are implicitly included in the SPARC/CCMI CMIP6 Ozone Database for historical simulations, which is derived from transient chemistry–climate model simulations and has been developed for climate models that do not calculate ozone interactively. CMIP6 models without chemistry that perform a preindustrial control simulation with time-varying solar forcing will need to use a modified version of the SPARC/CCMI Ozone Database that includes solar variability. CMIP6 models with interactive chemistry are also encouraged to use the particle forcing datasets, which will allow the potential long-term effects of particles to be addressed for the first time. The consideration of particle forcing has been shown to significantly improve the representation of reactive nitrogen and ozone variability in the polar middle atmosphere, eventually resulting in further improvements in the representation of solar climate variability in global models.
    Type of Medium: Online Resource
    ISSN: 1991-9603
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2017
    detail.hit.zdb_id: 2456725-5
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  • 8
    Online Resource
    Online Resource
    Copernicus GmbH ; 2019
    In:  Atmospheric Measurement Techniques Vol. 12, No. 2 ( 2019-03-01), p. 1375-1392
    In: Atmospheric Measurement Techniques, Copernicus GmbH, Vol. 12, No. 2 ( 2019-03-01), p. 1375-1392
    Abstract: Abstract. The Ku-band microwave frequencies (10.70–14.25 GHz) overlap emissions from ozone (O3) at 11.072 GHz and hydroxyl radical (OH) at 13.441 GHz. These important chemical species in the polar middle atmosphere respond strongly to high-latitude geomagnetic activity associated with space weather. Atmospheric model calculations predict that energetic electron precipitation (EEP) driven by magnetospheric substorms produces large changes in polar mesospheric O3 and OH. The EEP typically peaks at geomagnetic latitudes of ∼65∘ and evolves rapidly with time longitudinally and over the geomagnetic latitude range 60–80∘. Previous atmospheric modelling studies have shown that during substorms OH abundance can increase by more than an order of magnitude at 64–84 km and mesospheric O3 losses can exceed 50 %. In this work, an atmospheric simulation and retrieval study has been performed to determine the requirements for passive microwave radiometers capable of measuring diurnal variations in O3 and OH profiles from high-latitude Northern Hemisphere and Antarctic locations to verify model predictions. We show that, for a 11.072 GHz radiometer making 6 h spectral measurements with 10 kHz frequency resolution and root-mean-square baseline noise of 1 mK, O3 could be profiled over 8×10-4–0.22 hPa (∼98–58 km) with 10–17 km height resolution and ∼1 ppmv uncertainty. For the equivalent 13.441 GHz measurements with vertical sensor polarisation, OH could be profiled over 3×10-3–0.29 hPa (∼90–56 km) with 10–17 km height resolution and ∼3 ppbv uncertainty. The proposed observations would be highly applicable to studies of EEP, atmospheric dynamics, planetary-scale circulation, chemical transport, and the representation of these processes in polar and global climate models. Such observations would provide a relatively low-cost alternative to increasingly sparse satellite measurements of the polar middle atmosphere, extending long-term data records and also providing “ground truth” calibration data.
    Type of Medium: Online Resource
    ISSN: 1867-8548
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2019
    detail.hit.zdb_id: 2505596-3
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  • 9
    In: Geoscientific Model Development, Copernicus GmbH, Vol. 9, No. 9 ( 2016-09-12), p. 3123-3136
    Abstract: Abstract. This study presents a new ion–neutral chemical model coupled into the Whole Atmosphere Community Climate Model (WACCM). The ionospheric D-region (altitudes ∼  50–90 km) chemistry is based on the Sodankylä Ion Chemistry (SIC) model, a one-dimensional model containing 307 ion–neutral and ion recombination, 16 photodissociation and 7 photoionization reactions of neutral species, positive and negative ions, and electrons. The SIC mechanism was reduced using the simulation error minimization connectivity method (SEM-CM) to produce a reaction scheme of 181 ion–molecule reactions of 181 ion–molecule reactions of 27 positive and 18 negative ions. This scheme describes the concentration profiles at altitudes between 20 km and 120 km of a set of major neutral species (HNO3, O3, H2O2, NO, NO2, HO2, OH, N2O5) and ions (O2+, O4+, NO+, NO+(H2O), O2+(H2O), H+(H2O), H+(H2O)2, H+(H2O)3, H+(H2O)4, O3−, NO2−, O−, O2, OH−, O2−(H2O), O2−(H2O)2, O4−, CO3−, CO3−(H2O), CO4−, HCO3−, NO2−, NO3−, NO3−(H2O), NO3−(H2O)2, NO3−(HNO3), NO3−(HNO3)2, Cl−, ClO−), which agree with the full SIC mechanism within a 5 % tolerance. Four 3-D model simulations were then performed, using the impact of the January 2005 solar proton event (SPE) on D-region HOx and NOx chemistry as a test case of four different model versions: the standard WACCM (no negative ions and a very limited set of positive ions); WACCM-SIC (standard WACCM with the full SIC chemistry of positive and negative ions); WACCM-D (standard WACCM with a heuristic reduction of the SIC chemistry, recently used to examine HNO3 formation following an SPE); and WACCM-rSIC (standard WACCM with a reduction of SIC chemistry using the SEM-CM method). The standard WACCM misses the HNO3 enhancement during the SPE, while the full and reduced model versions predict significant NOx, HOx and HNO3 enhancements in the mesosphere during solar proton events. The SEM-CM reduction also identifies the important ion–molecule reactions that affect the partitioning of odd nitrogen (NOx), odd hydrogen (HOx) and O3 in the stratosphere and mesosphere.
    Type of Medium: Online Resource
    ISSN: 1991-9603
    Language: English
    Publisher: Copernicus GmbH
    Publication Date: 2016
    detail.hit.zdb_id: 2456725-5
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  • 10
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2013
    In:  Journal of Geophysical Research: Space Physics Vol. 118, No. 12 ( 2013-12), p. 7874-7885
    In: Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 118, No. 12 ( 2013-12), p. 7874-7885
    Abstract: Polar mesospheric NO increases during small recurrent geomagnetic storms Enhanced NO observed at 65–80 km is due to 〉 30 keV electron precipitation Horizontal and vertical transport redistributes NO in the polar winter
    Type of Medium: Online Resource
    ISSN: 2169-9380 , 2169-9402
    URL: Issue
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2013
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094181-7
    SSG: 16,13
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