ATProto Browser

Record data

{
  "uri": "at://did:plc:vorphoi2cdns5s4hqxu54smw/app.bsky.feed.post/3lmuphvnn7k2x",
  "cid": "bafyreiakeuoy6xjgibieyh76h3xgsjibynjunwitsj57bv7qj3ffqya7dy",
  "value": {
    "text": "What is this?\n\"Variations in the solar wind cause changes in electric currents that flow in the magnetosphere and ionosphere. The associated changes in the magnetic field can be observed using\n magnetometers on the\n ground.\"\nagupubs.onlinelibrary.wiley.com/doi/10.1029/...",
    "$type": "app.bsky.feed.post",
    "embed": {
      "$type": "app.bsky.embed.external",
      "external": {
        "uri": "https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022GL098860",
        "thumb": {
          "$type": "blob",
          "ref": {
            "$link": "bafkreibmrwzrqjdsx6tkquywlmjshibfmgi2azzjbaml6gdk2zr4hn32ti"
          },
          "mimeType": "image/jpeg",
          "size": 142906
        },
        "title": "Geomagnetic Activity Index Hpo",
        "description": "New Kp-like planetary geomagnetic activity indices, Hpo, are presented  Hourly (Hp60) and half-hourly (Hp30) indices are available from GFZ website  Hpo indices are open-ended without the upper li..."
      }
    },
    "langs": [
      "en"
    ],
    "reply": {
      "root": {
        "cid": "bafyreiecyrytmkvgsicfc4hww4ewccaygzzrieypnbkki6pjzg6cowiqba",
        "uri": "at://did:plc:rfh2f5pq3oxphxxoaatw664x/app.bsky.feed.post/3lmun52ikn22p"
      },
      "parent": {
        "cid": "bafyreiecyrytmkvgsicfc4hww4ewccaygzzrieypnbkki6pjzg6cowiqba",
        "uri": "at://did:plc:rfh2f5pq3oxphxxoaatw664x/app.bsky.feed.post/3lmun52ikn22p"
      }
    },
    "facets": [
      {
        "index": {
          "byteEnd": 272,
          "byteStart": 225
        },
        "features": [
          {
            "uri": "https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2022GL098860",
            "$type": "app.bsky.richtext.facet#link"
          }
        ]
      }
    ],
    "createdAt": "2025-04-15T18:30:08.577Z"
  }
}