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The Android Open Source Project9066cfe2009-03-03 19:31:44 -08001/*
2 * Copyright (C) 2009 The Android Open Source Project
3 *
4 * Licensed under the Apache License, Version 2.0 (the "License");
5 * you may not use this file except in compliance with the License.
6 * You may obtain a copy of the License at
7 *
8 * http://www.apache.org/licenses/LICENSE-2.0
9 *
10 * Unless required by applicable law or agreed to in writing, software
11 * distributed under the License is distributed on an "AS IS" BASIS,
12 * WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
13 * See the License for the specific language governing permissions and
14 * limitations under the License.
15 */
16
17package android.hardware;
18
19import java.util.GregorianCalendar;
20
21/**
Scott Main8edad6f2012-03-09 10:55:50 -080022 * Estimates magnetic field at a given point on
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080023 * Earth, and in particular, to compute the magnetic declination from true
24 * north.
25 *
26 * <p>This uses the World Magnetic Model produced by the United States National
27 * Geospatial-Intelligence Agency. More details about the model can be found at
28 * <a href="http://www.ngdc.noaa.gov/geomag/WMM/DoDWMM.shtml">http://www.ngdc.noaa.gov/geomag/WMM/DoDWMM.shtml</a>.
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030029 * This class currently uses WMM-2010 which is valid until 2015, but should
30 * produce acceptable results for several years after that. Future versions of
31 * Android may use a newer version of the model.
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080032 */
33public class GeomagneticField {
34 // The magnetic field at a given point, in nonoteslas in geodetic
35 // coordinates.
36 private float mX;
37 private float mY;
38 private float mZ;
39
40 // Geocentric coordinates -- set by computeGeocentricCoordinates.
41 private float mGcLatitudeRad;
42 private float mGcLongitudeRad;
43 private float mGcRadiusKm;
44
45 // Constants from WGS84 (the coordinate system used by GPS)
46 static private final float EARTH_SEMI_MAJOR_AXIS_KM = 6378.137f;
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030047 static private final float EARTH_SEMI_MINOR_AXIS_KM = 6356.7523142f;
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080048 static private final float EARTH_REFERENCE_RADIUS_KM = 6371.2f;
49
50 // These coefficients and the formulae used below are from:
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030051 // NOAA Technical Report: The US/UK World Magnetic Model for 2010-2015
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080052 static private final float[][] G_COEFF = new float[][] {
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030053 { 0.0f },
54 { -29496.6f, -1586.3f },
55 { -2396.6f, 3026.1f, 1668.6f },
56 { 1340.1f, -2326.2f, 1231.9f, 634.0f },
57 { 912.6f, 808.9f, 166.7f, -357.1f, 89.4f },
58 { -230.9f, 357.2f, 200.3f, -141.1f, -163.0f, -7.8f },
59 { 72.8f, 68.6f, 76.0f, -141.4f, -22.8f, 13.2f, -77.9f },
60 { 80.5f, -75.1f, -4.7f, 45.3f, 13.9f, 10.4f, 1.7f, 4.9f },
61 { 24.4f, 8.1f, -14.5f, -5.6f, -19.3f, 11.5f, 10.9f, -14.1f, -3.7f },
62 { 5.4f, 9.4f, 3.4f, -5.2f, 3.1f, -12.4f, -0.7f, 8.4f, -8.5f, -10.1f },
63 { -2.0f, -6.3f, 0.9f, -1.1f, -0.2f, 2.5f, -0.3f, 2.2f, 3.1f, -1.0f, -2.8f },
64 { 3.0f, -1.5f, -2.1f, 1.7f, -0.5f, 0.5f, -0.8f, 0.4f, 1.8f, 0.1f, 0.7f, 3.8f },
65 { -2.2f, -0.2f, 0.3f, 1.0f, -0.6f, 0.9f, -0.1f, 0.5f, -0.4f, -0.4f, 0.2f, -0.8f, 0.0f } };
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080066
67 static private final float[][] H_COEFF = new float[][] {
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030068 { 0.0f },
69 { 0.0f, 4944.4f },
70 { 0.0f, -2707.7f, -576.1f },
71 { 0.0f, -160.2f, 251.9f, -536.6f },
72 { 0.0f, 286.4f, -211.2f, 164.3f, -309.1f },
73 { 0.0f, 44.6f, 188.9f, -118.2f, 0.0f, 100.9f },
74 { 0.0f, -20.8f, 44.1f, 61.5f, -66.3f, 3.1f, 55.0f },
75 { 0.0f, -57.9f, -21.1f, 6.5f, 24.9f, 7.0f, -27.7f, -3.3f },
76 { 0.0f, 11.0f, -20.0f, 11.9f, -17.4f, 16.7f, 7.0f, -10.8f, 1.7f },
77 { 0.0f, -20.5f, 11.5f, 12.8f, -7.2f, -7.4f, 8.0f, 2.1f, -6.1f, 7.0f },
78 { 0.0f, 2.8f, -0.1f, 4.7f, 4.4f, -7.2f, -1.0f, -3.9f, -2.0f, -2.0f, -8.3f },
79 { 0.0f, 0.2f, 1.7f, -0.6f, -1.8f, 0.9f, -0.4f, -2.5f, -1.3f, -2.1f, -1.9f, -1.8f },
80 { 0.0f, -0.9f, 0.3f, 2.1f, -2.5f, 0.5f, 0.6f, 0.0f, 0.1f, 0.3f, -0.9f, -0.2f, 0.9f } };
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080081
82 static private final float[][] DELTA_G = new float[][] {
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030083 { 0.0f },
84 { 11.6f, 16.5f },
85 { -12.1f, -4.4f, 1.9f },
86 { 0.4f, -4.1f, -2.9f, -7.7f },
87 { -1.8f, 2.3f, -8.7f, 4.6f, -2.1f },
88 { -1.0f, 0.6f, -1.8f, -1.0f, 0.9f, 1.0f },
89 { -0.2f, -0.2f, -0.1f, 2.0f, -1.7f, -0.3f, 1.7f },
90 { 0.1f, -0.1f, -0.6f, 1.3f, 0.4f, 0.3f, -0.7f, 0.6f },
91 { -0.1f, 0.1f, -0.6f, 0.2f, -0.2f, 0.3f, 0.3f, -0.6f, 0.2f },
92 { 0.0f, -0.1f, 0.0f, 0.3f, -0.4f, -0.3f, 0.1f, -0.1f, -0.4f, -0.2f },
93 { 0.0f, 0.0f, -0.1f, 0.2f, 0.0f, -0.1f, -0.2f, 0.0f, -0.1f, -0.2f, -0.2f },
94 { 0.0f, 0.0f, 0.0f, 0.1f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, -0.1f, 0.0f },
95 { 0.0f, 0.0f, 0.1f, 0.1f, -0.1f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, -0.1f, 0.1f } };
The Android Open Source Project9066cfe2009-03-03 19:31:44 -080096
97 static private final float[][] DELTA_H = new float[][] {
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -030098 { 0.0f },
99 { 0.0f, -25.9f },
100 { 0.0f, -22.5f, -11.8f },
101 { 0.0f, 7.3f, -3.9f, -2.6f },
102 { 0.0f, 1.1f, 2.7f, 3.9f, -0.8f },
103 { 0.0f, 0.4f, 1.8f, 1.2f, 4.0f, -0.6f },
104 { 0.0f, -0.2f, -2.1f, -0.4f, -0.6f, 0.5f, 0.9f },
105 { 0.0f, 0.7f, 0.3f, -0.1f, -0.1f, -0.8f, -0.3f, 0.3f },
106 { 0.0f, -0.1f, 0.2f, 0.4f, 0.4f, 0.1f, -0.1f, 0.4f, 0.3f },
107 { 0.0f, 0.0f, -0.2f, 0.0f, -0.1f, 0.1f, 0.0f, -0.2f, 0.3f, 0.2f },
108 { 0.0f, 0.1f, -0.1f, 0.0f, -0.1f, -0.1f, 0.0f, -0.1f, -0.2f, 0.0f, -0.1f },
109 { 0.0f, 0.0f, 0.1f, 0.0f, 0.1f, 0.0f, 0.1f, 0.0f, -0.1f, -0.1f, 0.0f, -0.1f },
110 { 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, 0.1f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f, 0.0f } };
The Android Open Source Project9066cfe2009-03-03 19:31:44 -0800111
112 static private final long BASE_TIME =
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -0300113 new GregorianCalendar(2010, 1, 1).getTimeInMillis();
The Android Open Source Project9066cfe2009-03-03 19:31:44 -0800114
115 // The ratio between the Gauss-normalized associated Legendre functions and
116 // the Schmid quasi-normalized ones. Compute these once staticly since they
117 // don't depend on input variables at all.
118 static private final float[][] SCHMIDT_QUASI_NORM_FACTORS =
119 computeSchmidtQuasiNormFactors(G_COEFF.length);
120
121 /**
122 * Estimate the magnetic field at a given point and time.
123 *
124 * @param gdLatitudeDeg
125 * Latitude in WGS84 geodetic coordinates -- positive is east.
126 * @param gdLongitudeDeg
127 * Longitude in WGS84 geodetic coordinates -- positive is north.
128 * @param altitudeMeters
129 * Altitude in WGS84 geodetic coordinates, in meters.
130 * @param timeMillis
131 * Time at which to evaluate the declination, in milliseconds
132 * since January 1, 1970. (approximate is fine -- the declination
133 * changes very slowly).
134 */
135 public GeomagneticField(float gdLatitudeDeg,
136 float gdLongitudeDeg,
137 float altitudeMeters,
138 long timeMillis) {
139 final int MAX_N = G_COEFF.length; // Maximum degree of the coefficients.
140
141 // We don't handle the north and south poles correctly -- pretend that
142 // we're not quite at them to avoid crashing.
143 gdLatitudeDeg = Math.min(90.0f - 1e-5f,
144 Math.max(-90.0f + 1e-5f, gdLatitudeDeg));
145 computeGeocentricCoordinates(gdLatitudeDeg,
146 gdLongitudeDeg,
147 altitudeMeters);
148
149 assert G_COEFF.length == H_COEFF.length;
150
151 // Note: LegendreTable computes associated Legendre functions for
152 // cos(theta). We want the associated Legendre functions for
153 // sin(latitude), which is the same as cos(PI/2 - latitude), except the
154 // derivate will be negated.
155 LegendreTable legendre =
156 new LegendreTable(MAX_N - 1,
157 (float) (Math.PI / 2.0 - mGcLatitudeRad));
158
159 // Compute a table of (EARTH_REFERENCE_RADIUS_KM / radius)^n for i in
160 // 0..MAX_N-2 (this is much faster than calling Math.pow MAX_N+1 times).
161 float[] relativeRadiusPower = new float[MAX_N + 2];
162 relativeRadiusPower[0] = 1.0f;
163 relativeRadiusPower[1] = EARTH_REFERENCE_RADIUS_KM / mGcRadiusKm;
164 for (int i = 2; i < relativeRadiusPower.length; ++i) {
165 relativeRadiusPower[i] = relativeRadiusPower[i - 1] *
166 relativeRadiusPower[1];
167 }
168
169 // Compute tables of sin(lon * m) and cos(lon * m) for m = 0..MAX_N --
170 // this is much faster than calling Math.sin and Math.com MAX_N+1 times.
171 float[] sinMLon = new float[MAX_N];
172 float[] cosMLon = new float[MAX_N];
173 sinMLon[0] = 0.0f;
174 cosMLon[0] = 1.0f;
175 sinMLon[1] = (float) Math.sin(mGcLongitudeRad);
176 cosMLon[1] = (float) Math.cos(mGcLongitudeRad);
177
178 for (int m = 2; m < MAX_N; ++m) {
179 // Standard expansions for sin((m-x)*theta + x*theta) and
180 // cos((m-x)*theta + x*theta).
181 int x = m >> 1;
182 sinMLon[m] = sinMLon[m-x] * cosMLon[x] + cosMLon[m-x] * sinMLon[x];
183 cosMLon[m] = cosMLon[m-x] * cosMLon[x] - sinMLon[m-x] * sinMLon[x];
184 }
185
186 float inverseCosLatitude = 1.0f / (float) Math.cos(mGcLatitudeRad);
187 float yearsSinceBase =
188 (timeMillis - BASE_TIME) / (365f * 24f * 60f * 60f * 1000f);
189
190 // We now compute the magnetic field strength given the geocentric
191 // location. The magnetic field is the derivative of the potential
192 // function defined by the model. See NOAA Technical Report: The US/UK
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -0300193 // World Magnetic Model for 2010-2015 for the derivation.
The Android Open Source Project9066cfe2009-03-03 19:31:44 -0800194 float gcX = 0.0f; // Geocentric northwards component.
195 float gcY = 0.0f; // Geocentric eastwards component.
196 float gcZ = 0.0f; // Geocentric downwards component.
197
198 for (int n = 1; n < MAX_N; n++) {
199 for (int m = 0; m <= n; m++) {
200 // Adjust the coefficients for the current date.
201 float g = G_COEFF[n][m] + yearsSinceBase * DELTA_G[n][m];
202 float h = H_COEFF[n][m] + yearsSinceBase * DELTA_H[n][m];
203
204 // Negative derivative with respect to latitude, divided by
205 // radius. This looks like the negation of the version in the
206 // NOAA Techincal report because that report used
207 // P_n^m(sin(theta)) and we use P_n^m(cos(90 - theta)), so the
208 // derivative with respect to theta is negated.
209 gcX += relativeRadiusPower[n+2]
210 * (g * cosMLon[m] + h * sinMLon[m])
211 * legendre.mPDeriv[n][m]
212 * SCHMIDT_QUASI_NORM_FACTORS[n][m];
213
214 // Negative derivative with respect to longitude, divided by
215 // radius.
216 gcY += relativeRadiusPower[n+2] * m
217 * (g * sinMLon[m] - h * cosMLon[m])
218 * legendre.mP[n][m]
219 * SCHMIDT_QUASI_NORM_FACTORS[n][m]
220 * inverseCosLatitude;
221
222 // Negative derivative with respect to radius.
223 gcZ -= (n + 1) * relativeRadiusPower[n+2]
224 * (g * cosMLon[m] + h * sinMLon[m])
225 * legendre.mP[n][m]
226 * SCHMIDT_QUASI_NORM_FACTORS[n][m];
227 }
228 }
229
230 // Convert back to geodetic coordinates. This is basically just a
231 // rotation around the Y-axis by the difference in latitudes between the
232 // geocentric frame and the geodetic frame.
233 double latDiffRad = Math.toRadians(gdLatitudeDeg) - mGcLatitudeRad;
234 mX = (float) (gcX * Math.cos(latDiffRad)
235 + gcZ * Math.sin(latDiffRad));
236 mY = gcY;
237 mZ = (float) (- gcX * Math.sin(latDiffRad)
238 + gcZ * Math.cos(latDiffRad));
239 }
240
241 /**
242 * @return The X (northward) component of the magnetic field in nanoteslas.
243 */
244 public float getX() {
245 return mX;
246 }
247
248 /**
249 * @return The Y (eastward) component of the magnetic field in nanoteslas.
250 */
251 public float getY() {
252 return mY;
253 }
254
255 /**
256 * @return The Z (downward) component of the magnetic field in nanoteslas.
257 */
258 public float getZ() {
259 return mZ;
260 }
261
262 /**
263 * @return The declination of the horizontal component of the magnetic
264 * field from true north, in degrees (i.e. positive means the
265 * magnetic field is rotated east that much from true north).
266 */
267 public float getDeclination() {
268 return (float) Math.toDegrees(Math.atan2(mY, mX));
269 }
270
271 /**
272 * @return The inclination of the magnetic field in degrees -- positive
273 * means the magnetic field is rotated downwards.
274 */
275 public float getInclination() {
276 return (float) Math.toDegrees(Math.atan2(mZ,
277 getHorizontalStrength()));
278 }
279
280 /**
281 * @return Horizontal component of the field strength in nonoteslas.
282 */
283 public float getHorizontalStrength() {
Neil Fuller33253a42014-10-01 11:55:10 +0100284 return (float) Math.hypot(mX, mY);
The Android Open Source Project9066cfe2009-03-03 19:31:44 -0800285 }
286
287 /**
288 * @return Total field strength in nanoteslas.
289 */
290 public float getFieldStrength() {
291 return (float) Math.sqrt(mX * mX + mY * mY + mZ * mZ);
292 }
293
294 /**
295 * @param gdLatitudeDeg
296 * Latitude in WGS84 geodetic coordinates.
297 * @param gdLongitudeDeg
298 * Longitude in WGS84 geodetic coordinates.
299 * @param altitudeMeters
300 * Altitude above sea level in WGS84 geodetic coordinates.
301 * @return Geocentric latitude (i.e. angle between closest point on the
302 * equator and this point, at the center of the earth.
303 */
304 private void computeGeocentricCoordinates(float gdLatitudeDeg,
305 float gdLongitudeDeg,
306 float altitudeMeters) {
307 float altitudeKm = altitudeMeters / 1000.0f;
308 float a2 = EARTH_SEMI_MAJOR_AXIS_KM * EARTH_SEMI_MAJOR_AXIS_KM;
309 float b2 = EARTH_SEMI_MINOR_AXIS_KM * EARTH_SEMI_MINOR_AXIS_KM;
310 double gdLatRad = Math.toRadians(gdLatitudeDeg);
311 float clat = (float) Math.cos(gdLatRad);
312 float slat = (float) Math.sin(gdLatRad);
313 float tlat = slat / clat;
314 float latRad =
315 (float) Math.sqrt(a2 * clat * clat + b2 * slat * slat);
316
317 mGcLatitudeRad = (float) Math.atan(tlat * (latRad * altitudeKm + b2)
318 / (latRad * altitudeKm + a2));
319
320 mGcLongitudeRad = (float) Math.toRadians(gdLongitudeDeg);
321
322 float radSq = altitudeKm * altitudeKm
323 + 2 * altitudeKm * (float) Math.sqrt(a2 * clat * clat +
324 b2 * slat * slat)
325 + (a2 * a2 * clat * clat + b2 * b2 * slat * slat)
326 / (a2 * clat * clat + b2 * slat * slat);
327 mGcRadiusKm = (float) Math.sqrt(radSq);
328 }
329
330
331 /**
332 * Utility class to compute a table of Gauss-normalized associated Legendre
333 * functions P_n^m(cos(theta))
334 */
335 static private class LegendreTable {
336 // These are the Gauss-normalized associated Legendre functions -- that
337 // is, they are normal Legendre functions multiplied by
338 // (n-m)!/(2n-1)!! (where (2n-1)!! = 1*3*5*...*2n-1)
339 public final float[][] mP;
340
341 // Derivative of mP, with respect to theta.
342 public final float[][] mPDeriv;
343
344 /**
345 * @param maxN
346 * The maximum n- and m-values to support
347 * @param thetaRad
348 * Returned functions will be Gauss-normalized
349 * P_n^m(cos(thetaRad)), with thetaRad in radians.
350 */
351 public LegendreTable(int maxN, float thetaRad) {
352 // Compute the table of Gauss-normalized associated Legendre
353 // functions using standard recursion relations. Also compute the
354 // table of derivatives using the derivative of the recursion
355 // relations.
356 float cos = (float) Math.cos(thetaRad);
357 float sin = (float) Math.sin(thetaRad);
358
359 mP = new float[maxN + 1][];
360 mPDeriv = new float[maxN + 1][];
361 mP[0] = new float[] { 1.0f };
362 mPDeriv[0] = new float[] { 0.0f };
363 for (int n = 1; n <= maxN; n++) {
John Spurlock8a985d22014-02-25 09:40:05 -0500364 mP[n] = new float[n + 1];
The Android Open Source Project9066cfe2009-03-03 19:31:44 -0800365 mPDeriv[n] = new float[n + 1];
366 for (int m = 0; m <= n; m++) {
367 if (n == m) {
368 mP[n][m] = sin * mP[n - 1][m - 1];
369 mPDeriv[n][m] = cos * mP[n - 1][m - 1]
370 + sin * mPDeriv[n - 1][m - 1];
371 } else if (n == 1 || m == n - 1) {
372 mP[n][m] = cos * mP[n - 1][m];
373 mPDeriv[n][m] = -sin * mP[n - 1][m]
374 + cos * mPDeriv[n - 1][m];
375 } else {
376 assert n > 1 && m < n - 1;
377 float k = ((n - 1) * (n - 1) - m * m)
378 / (float) ((2 * n - 1) * (2 * n - 3));
379 mP[n][m] = cos * mP[n - 1][m] - k * mP[n - 2][m];
380 mPDeriv[n][m] = -sin * mP[n - 1][m]
381 + cos * mPDeriv[n - 1][m] - k * mPDeriv[n - 2][m];
382 }
383 }
384 }
385 }
386 }
387
388 /**
389 * Compute the ration between the Gauss-normalized associated Legendre
390 * functions and the Schmidt quasi-normalized version. This is equivalent to
391 * sqrt((m==0?1:2)*(n-m)!/(n+m!))*(2n-1)!!/(n-m)!
392 */
393 private static float[][] computeSchmidtQuasiNormFactors(int maxN) {
394 float[][] schmidtQuasiNorm = new float[maxN + 1][];
395 schmidtQuasiNorm[0] = new float[] { 1.0f };
396 for (int n = 1; n <= maxN; n++) {
397 schmidtQuasiNorm[n] = new float[n + 1];
398 schmidtQuasiNorm[n][0] =
399 schmidtQuasiNorm[n - 1][0] * (2 * n - 1) / (float) n;
400 for (int m = 1; m <= n; m++) {
401 schmidtQuasiNorm[n][m] = schmidtQuasiNorm[n][m - 1]
402 * (float) Math.sqrt((n - m + 1) * (m == 1 ? 2 : 1)
403 / (float) (n + m));
404 }
405 }
406 return schmidtQuasiNorm;
407 }
Rodrigo Damazio Bovendorp9119caa2010-03-15 21:19:59 -0300408}