MediaWiki API result

{
    "batchcomplete": "",
    "continue": {
        "gapcontinue": "Solar-Wind_Drivers_or_Internal_Magnetospheric_Processes",
        "continue": "gapcontinue||"
    },
    "warnings": {
        "main": {
            "*": "Subscribe to the mediawiki-api-announce mailing list at <https://lists.wikimedia.org/mailman/listinfo/mediawiki-api-announce> for notice of API deprecations and breaking changes."
        },
        "revisions": {
            "*": "Because \"rvslots\" was not specified, a legacy format has been used for the output. This format is deprecated, and in the future the new format will always be used."
        }
    },
    "query": {
        "pages": {
            "41": {
                "pageid": 41,
                "ns": 0,
                "title": "SEPs from Heliosphere to Magnetosphere",
                "revisions": [
                    {
                        "contentformat": "text/x-wiki",
                        "contentmodel": "wikitext",
                        "*": "'''Candidate SHINE co-convener: Janet Luhmann <jgluhman [at] ssl.berkeley.edu>'''\n\n'''Candidate GEM co-convener: Mary Hudson <mary.hudson [at] dartmouth.edu>''' \n\nA brief but productive discussion of the problem of SEPs (Solar\nEnergetic Particles) from their production in the heliosphere to\ntheir geospace effects, was held on Thursday, June 26. This is\na particularly rich and appropriate GEM/SHINE topical\narea because it involves connecting a chain of processes\noccurring in the solar corona and interplanetary medium to responses\nin the middle atmosphere, via the magnetosphere.\nThe large solar proton events that are of most interest\nwere the main focus of the discussion, which was kicked off\nwith an overview of the heliospheric end by David Lario (JHUAPL).\nDavid described the still outstanding problems of a lack of\nunderstanding of the details of the particle production, energization\nand transport. This was followed by a more specific discussion\nby David Ruffolo (Mahidol Univ.) of the most energetic of SEP events,\nGLEs or Ground Level Events, which are detected on the ground by\nNeutron Monitors. The major events which represent the deepest\npenetrations of SEP event effects typically occur only once or\ntwice per solar cycle, and the reason for their particularly\ngreat fluxes of protons at high energies reaching into the GeV\nrange is still a subject of investigation. These events have\ncertain properties such as prompt arrival and high antisunward,\nfield-aligned anisotropies that affect the way they are\nperceived on the ground. Brian Kress (Dartmouth) spoke on\nthe magnetospheric access of the SEPs, and coincidentally, on\nthe effect of the particle flux anisotropy on access to\nhigh latitudes along open field lines. Simulations of the proton\naccess in MHD magnetosphere models show geomagnetic cutoffs will appear\ndifferent in measurements when significant anisotropies exist.\nThus ground (and LEO and atmosphere) exposure to SEP effects for the\nmost energetic events is somewhat less predictable using cutoffs\ncomputed for isotropic incident fluxes. Tamitha Mulligan (Aerospace)\nspoke on several recent large SEP events observed in both the\nheliosphere and magnetosphere. She showed that there were features\nin the magnetospheric time profiles not present in the interplanetary\ntime profiles, suggesting magnetospheric modulation of the intrinsic\ntime profiles, perhaps. Finally, Stan Solomon (HAO) spoke on the\nrecent modeling of SEP event effects in the atmosphere using the\nWACCM (Whole Atmosphere Community Climate Model). This model can\ntrace the 3D dynamical and chemical effects of SEP events from the\ntop of the thermosphere to the ground. Stan showed some results\nfrom Jackman and coworkers for some previous large proton events.\nThe NO and ozone chemistry effects can be seen to last for months\nafter the event, and to make their way well into the middle atmosphere-\nand occasionally into the stratosphere. The potential for tracing\nthis full chain of SEP physics from end to end has never been greater."
                    }
                ]
            },
            "51": {
                "pageid": 51,
                "ns": 0,
                "title": "Small-Scale Structure in the Solar Wind and Its Effect on Earth",
                "revisions": [
                    {
                        "contentformat": "text/x-wiki",
                        "contentmodel": "wikitext",
                        "*": "'''SHINE co-convener: Joe Borovsky <jborovsky @ lanl.gov>''' \n\n'''GEM co-convener: Beniot Lavraud <Benoit.Lavraud @ cesr.fr>''' \n\nOn Tuesday June 24, between 1:30 \u2013 3:30 pm, was held one of the several Coordinated GEM-SHINE sessions. This session was devoted to \u201cSmall scale structure in the solar wind and its effect on Earth\u201d. It was proposed by J. E. Borovsky and chaired B. Lavraud and J. Steinberg. The aim of the session was to promote discussions between experts that address topics which, though often studied separately, all eventually act together in the driving magnetospheric activity. \n\nThe topics that were addressed during the session, and the experts that discussed those, included:\n\n- The propagation of solar wind structures in the solar wind;\n(Dan Weimer, Chris Russell)\n\n- Periodic variations and turbulence in solar wind;\n(Nicky Viall, David Ruffolo)\n\n- Magnetospheric reaction to solar wind structures (e.g., substorms);\n(Nicky Viall, Tung-Shin Hsu, Raluca Ilie)\n\n- Structure during High-Speed Streams and influence on Earth.\n(Steinberg for Borovsky)\n\n- Current sheets hitting Earth and foreshock influence;\n(Xochitl Blanco-Cano, Larry Lyons)"
                    }
                ]
            }
        }
    }
}