Search Results - "Van der Swaluw, E."

Bjerknes Compensation at High Northern Latitudes: The Ocean Forcing the Atmosphere by van der Swaluw, E., Drijfhout, S. S., Hazeleger, W.

“…The mechanisms for Bjerknes compensation of heat transport variations through the atmosphere and ocean on decadal time scales are investigated, using data…”
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The X-Ray Structure of the Pulsar Bow Shock G189.22+2.90 in the Supernova Remnant IC 443 by Gaensler, B. M, Chatterjee, S, Slane, P. O, van der Swaluw, E, Camilo, F, Hughes, J. P

“…We present a deep observation with the Chandra X-Ray Observatory of the neutron star bow shock G189.22+2.90 in the supernova remnant (SNR) IC 443. Our data…”
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Proper-Motion Measurements of Pulsar B1951+32 in the Supernova Remnant CTB 80 by Migliazzo, J. M, Gaensler, B. M, Backer, D. C, Stappers, B. W, van der Swaluw, E, Strom, R. G

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Inferring Initial Spin Periods for Neutron Stars in Composite Remnants by van der Swaluw, E, Wu, Y

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Trends in ammonia measurements in the Netherlands over the period 1993–2014 by van Zanten, M.C., Wichink Kruit, R.J., Hoogerbrugge, R., Van der Swaluw, E., van Pul, W.A.J.

“…We present measurements of atmospheric concentrations of ammonia and ammonium in the Netherlands over the period 1993–2014 and measurements of wet deposition…”
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Implementation and evaluation of pH-dependent cloud chemistry and wet deposition in the chemical transport model REM-Calgrid by Banzhaf, S., Schaap, M., Kerschbaumer, A., Reimer, E., Stern, R., van der Swaluw, E., Builtjes, P.

“…The Chemistry Transport Model REM-Calgrid (RCG) has been improved by implementing an enhanced description of aqueous-phase chemistry and wet deposition…”
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A PROPER MOTION FOR THE PULSAR WIND NEBULA G359.23–0.82, THE “MOUSE,” ASSOCIATED WITH THE ENERGETIC RADIO PULSAR J1747–2958 by Hales, C A, Gaensler, B M, Chatterjee, S, van der Swaluw, E, Camilo, F

“…The 'Mouse' (PWN G359.23-0.82) is a spectacular bow shock pulsar wind nebula, powered by the radio pulsar J1747-2958. The pulsar and its nebula are presumed to…”
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The Mouse that Soared: High-Resolution X-Ray Imaging of the Pulsar-powered Bow Shock G359.23–0.82 by Gaensler, B. M, van der Swaluw, E, Camilo, F, Kaspi, V. M, Baganoff, F. K, Yusef-Zadeh, F, Manchester, R. N

“…We present an observation with the Chandra X-Ray Observatory of the unusual radio source G359.23-0.82 ("the Mouse"), along with updated radio timing data from…”
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Modelling the future distribution of ammonium nitrate concentrations in The Netherlands for 2020: The sensitivity to meteorological parameters by Williams, J.E., van der Swaluw, E., de Vries, W.J., Sauter, F.J., van Pul, W.A.J., Hoogerbrugge, R.

“…We present a parameterization developed to simulate Ammonium particle (NH4+) concentrations in the Operational Priority Substances (OPS) source-receptor model,…”
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The Duck Redux: An Improved Proper-Motion Upper Limit for the Pulsar B1757–24 near the Supernova Remnant G5.4-1.2 by Blazek, J. A, Gaensler, B. M, Chatterjee, S, van der Swaluw, E, Camilo, F, Stappers, B. W

“…"The Duck" is a complicated nonthermal radio system, consisting of the energetic radio pulsar B1757-24, its surrounding pulsar wind nebula G5.27-0.90, and the…”
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Do we really observe a bow shock in N157B...? by van der Swaluw, E

“…I present a model of a pulsar wind interacting with its associated supernova remnant. I will use the model to argue that one can explain the morphology of the…”
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MHD interaction of pulsar wind nebulae with SNRs and with the ISM by van der Swaluw, E.

“…In the late 1960s the discovery of the Crab pulsar in its associated supernova remnant, launched a new field in supernova remnant research: the study of…”
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Long-range and local air pollution: what can we learn from chemical speciation of particulate matter at paired sites? by Pandolfi, Marco, Mooibroek, Dennis, Hopke, Philip, van Pinxteren, Dominik, Querol, Xavier, Herrmann, Hartmut, Alastuey, Andrés, Favez, Olivier, Hüglin, Christoph, Perdrix, Esperanza, Riffault, Véronique, Sauvage, Stéphane, van der Swaluw, Eric, Tarasova, Oksana, Colette, Augustin

“…Here we report results of a detailed analysis of the urban and non-urban contributions to particulate matter (PM) concentrations and source contributions in…”
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Modelling trends in ammonia in the Netherlands over the period 1990–2014 by Wichink Kruit, R.J., Aben, J., de Vries, W., Sauter, F., van der Swaluw, E., van Zanten, M.C., van Pul, W.A.J.

“…This study investigates to what extent emissions of ammonia, physicochemical processes and meteorology affect the trend in the atmospheric ammonia in the…”
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Curriculum vitae of the LOTOS–EUROS (v2.0) chemistry transport model by Manders, Astrid M. M, Builtjes, Peter J. H, Curier, Lyana, Denier van der Gon, Hugo A. C, Hendriks, Carlijn, Jonkers, Sander, Kranenburg, Richard, Kuenen, Jeroen J. P, Segers, Arjo J, Timmermans, Renske M. A, Visschedijk, Antoon J. H, Wichink Kruit, Roy J, van Pul, W. Addo J, Sauter, Ferd J, van der Swaluw, Eric, Swart, Daan P. J, Douros, John, Eskes, Henk, van Meijgaard, Erik, van Ulft, Bert, van Velthoven, Peter, Banzhaf, Sabine, Mues, Andrea C, Stern, Rainer, Fu, Guangliang, Lu, Sha, Heemink, Arnold, van Velzen, Nils, Schaap, Martijn

“…The development and application of chemistry transport models has a long tradition. Within the Netherlands the LOTOS–EUROS model has been developed by a…”
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New Constraints on the Structure and Evolution of the Pulsar Wind Nebula 3C 58 by Slane, Patrick, Helfand, David J, van der Swaluw, Eric, Murray, Stephen S

“…We present an investigation of the spectral and spatial structure of the X-ray emission from 3C 58 based on a 350 ks observation with the Chandra X-ray…”
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A PROPER MOTION FOR THE PULSAR WIND NEBULA G359.23-0.82, THE MOUSE, ASSOCIATED WITH THE ENERGETIC RADIO PULSAR J 1747-2958 by HALES, C. A, GAENSLER, B. M, CHATTERJEE, S, VAN DER SWALUW, E, CAMILO, And F

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A Proper Motion for the Pulsar Wind Nebula G359.23–0.82, the by Hales, C. A, Gaensler, B. M, Chatterjee, S, van der Swaluw, E, Camilo, F

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A Proper Motion for the Pulsar Wind Nebula G359.23-0.82, "the Mouse," Associated with the Energetic Radio Pulsar J1747-2958 by Hales, C. A, Gaensler, B. M, Chatterjee, S, van der Swaluw, E, Camilo, F

“…Astrophys.J.706:1316-1322,2009 The "Mouse" (PWN G359.23-0.82) is a spectacular bow shock pulsar wind nebula, powered by the radio pulsar J1747-2958. The pulsar…”
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The nature of the X-ray halo of the plerion G21.5-0.9 unveiled by XMM-Newton and Chandra by Bocchino, F, van der Swaluw, E, Chevalier, R, Bandiera, R

“…The nature of the radio-quiet X-ray halo around the plerionic SNR G21.5-0.9 is under debate. On the basis of spatial and spectral analysis of a large Chandra…”
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