MediaWiki API result

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    "continue": {
        "gapcontinue": "Resonant_Magnetic_Perturbation",
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    "warnings": {
        "main": {
            "*": "Subscribe to the mediawiki-api-announce mailing list at <https://lists.wikimedia.org/postorius/lists/mediawiki-api-announce.lists.wikimedia.org/> for notice of API deprecations and breaking changes."
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            "*": "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."
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    "query": {
        "pages": {
            "564": {
                "pageid": 564,
                "ns": 0,
                "title": "Reconnection",
                "revisions": [
                    {
                        "contentformat": "text/x-wiki",
                        "contentmodel": "wikitext",
                        "*": "Magnetic reconnection refers to the breaking and reconnecting of oppositely directed magnetic field lines in a plasma. \nIn the process, magnetic field energy is converted to plasma kinetic and thermal energy. \n[[File:Reconnection.jpg|420px|thumb|right|Sketch of the reconnection process]]\n\n== See also ==\n* [[Wikipedia:Magnetic reconnection|Magnetic reconnection]]\n* [https://mrx.pppl.gov/Physics/physics.html What is magnetic reconnection?]\n* [[Sawtooth]]"
                    }
                ]
            },
            "365": {
                "pageid": 365,
                "ns": 0,
                "title": "Resistive timescale",
                "revisions": [
                    {
                        "contentformat": "text/x-wiki",
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                        "*": "The resistive timescale is the typical time for the diffusion of a magnetic field into a resistive plasma.\nBased on Faraday's Law,\n:<math>\\frac{\\partial \\vec B}{\\partial t} = -\\vec \\nabla \\times \\vec E,</math>\nOhm's Law,\n:<math>\\vec E = \\eta \\vec j,</math>\nwhere ''&eta;'' is the [[:Wikipedia:Spitzer_resistivity|resistivity]] (assumed homogeneous), and Amp\u00e8re's Law,\n:<math> \\vec \\nabla \\times \\vec B = \\mu_0 \\vec j,</math>\none immediately derives a diffusion type equation for the magnetic field:\n:<math>\\frac{\\partial \\vec B}{\\partial t} = -\\frac{\\eta}{\\mu_0} \\vec \\nabla \\times \\vec \\nabla \\times \\vec B = \\frac{\\eta}{\\mu_0} \\nabla^2 \\vec B,</math>\nsince \n: <math>\\vec \\nabla \\cdot \\vec B = 0.</math>\nFrom this, one can deduce the typical timescale\n:<math> \\tau_R \\simeq \\frac{\\mu_0 L^2}{\\eta}.</math>\nHere, ''L'' is the typical length scale of the problem, often taken equal to ''a'', the [[Toroidal coordinates|minor radius]] of the toroidal plasma.\n\n== See also ==\n\n* [[:Wikipedia:Lundquist number|Lundquist number]]"
                    }
                ]
            }
        }
    }
}