Selected quad for the lemma: cause_n

Word A	Word B	Word C	Word D	Occurrence	Frequency Band	MI	MI Band	Prominent
cause_n	bring_v	day_n	time_n	1,694	5	3.4053	3	false

Text snippets containing the quad

ID	Title	Author	Corrected Date of Publication (TCP Date of Publication)	STC	Words	Pages
A14624	The mariners mirrour wherin may playnly be seen the courses, heights, distances, depths, soundings, flouds and ebs, risings of lands, rocks, sands and shoalds, with the marks for th'entrings of the harbouroughs, havens and ports of the greatest part of Europe: their seueral traficks and commodities: together wth. the rules and instrume[n]ts of navigation. First made & set fourth in diuers exact sea-charts, by that famous nauigator Luke Wagenar of Enchuisen and now fitted with necessarie additions for the use of Englishmen by Anthony Ashley. Heerin also may be understood the exploits lately atchiued by the right Honorable the L. Admiral of Engla[n]d with her Maties. nauie and some former seruices don by that worthy knight Sr. Fra: Drake.; Spieghel der zeevaerdt. English	Waghenaer, Lucas Janszoon, 1534 or 5-1606.; Ashley, Anthony, Sir, 1551-1628.; Bry, Theodor de, 1528-1598, engraver.; Hondius, Jodocus, 1563-1612, engraver.; Ryther, Augustine, engraver.	1588 (1588)	STC 24931; ESTC S122236	118,075	186

3● 1 3● 20 2● 29 19 38 29 7 48 1606 11 24 8 46 22 22 23 21 13 3 21 1 41 19 13 28 18 23 43 1588 12 13 2 58 11 16 38 10 5 32 9 17 7 8 4 16 7 14 50   13 2 31 1 ●6 ●7 3● 30 10 58 29 2 7 28 16 38 27 5 24 26 17 1   14 20 20 23 19 11 29 18 4 0 17 21 29 16 14 8 16 5 8   15 10 2 11 8 14 23 7 5 0 6 21 26 5 15 59 5 10 25   16 28 23 41 25 10 18 26 23 38 24 15 50 23 10 25 23 5 46   17 17 15 10 15 22 51 14 8 25 13 20 28 12 11 33 12 5 10   18 7 8 3 5 15 38 3 23 14 3 8 21 1 19 22 1 ●1 ● 1 ●6 5 1595 19 26 7 38 24 16 3 23 0 44 22 9 41 20 20 4 20 6 57 A VVAIE TO FINDE OVT THE LEAPE YEERE WITHOVT eyther Calender or Ephemerides DIuide the yeeres of our Lord by 4. and if nothing remayne after the diuision that yeare is Leape yeare but if the number of 1. 2. or 3. shall remaine it signifieth what yeere it is after the Leape yeare As for example Take the yeare since the Natiuitie of Christ 1588. which beeing diuided by 4. nothing remayneth wherefore it is Leape yeare And the yeere 1589. the first after the Leape yeere The yeare 1590. the second the yeare 1591. the third But the yeare 1592. shall bee a Leape yeare againe and so forwards OF THE DECLINATION OF THE Sunne and the vse thereof FOr asmuch as for many and waighty causes ten daies are once for euer cut off from the yeare by certaine Monarchs of Europe as needlesse that thereby the Equinoctiall or Solstitiall pointes might bee brought to the same dayes of the moneth as of olde time they were in the time of the Nicene councel and so the 4. seasons of the yeare viz. the Spring Summer Haruest and VVinter begin on the same dayes as they were wont And furthermore as the appearances and suppositions of the 8. sphere do shew a manifest inequality in the greatnes of the sunne so in continuance of time as apparant an alteration is perceiued in his greatest obliquation For by the obseruations of Erarosthenes Hipparchus and Ptolomy of which the two first liued a little before the beginning of the Romaine Empire and the third a little after the greatest obliquation of the sunne was found to be almost euen with his vtmost declination so that in the time of Iulius Caesar and the beginning of the Romaine Empire the greatest was of 23. degrees and 52 minutes But afterward it decreased by little and little as plainly appeareth by the obseruations of Albaregnius and since by Arzahel the Spanyard Almeon Almanzor Prophatius the Ievve and many others which for this last hundred yeares by the diligent study and obseruing of George Purbachius Iohannes Regiomontanus Vernerus Copernicus c. is yet found still decreasing so that at this time it is well neare vpon the last and farthest poynt viz. in 23. degrees and 28. minutes or at least wanting a few seconds Therefore VVagener thought it not impertinent to set downe the table of the declination of the Sunne for the behoofe of all Pilots Shipmasters and all kinde of Saylers aswell according to the right course of the sunne as this apparant obliquation of our time hoping that he should doe therein that which should be acceptable and not vnprofitable vnto them But it hath since beene thought fitter for vs in England to follow our auncient and accustomed stile not acknowledging any such perfection of the Gregorian reformation ❧ OF THE VSE OF THE Table following for the Sunnes declination FIrst you must know whether it be a Leape yeare or the first second or third yeare after the Leape yeare and when you vnderstand the same entring the Table of that yeare you shall seeke out your purposed moneth and day in the toppe and side titles for the common Angle will shew the declination of the sunne for the same day northward from the 10. of March to the 13. of September and southward from the 13. of September to the 10. of March and these dayes are marked thus ✚ Now if you desire to knowe the latitude of any countrey or height of the Pole take the meridian height of the sunne by your Astrolabe or Crosse staffe and it will shewe the distance of the sunne from the Zenith or highest poynt And if the declination of the sunne be Northward the same day adde it to the distance of the sunne from the Zenith But contrarywise deduct it againe if the declination be Southward and you shall haue the latitude of that place or the altitude of the Pole As for example VVagener in the yeere 1583. the 21. of Ianuary tooke by Astrolabe at Enchuysen the meridian altitude of the sunne about 20. degrees and 50. minutes wherefore the distance thereof from the Zenith is neare 69. degrees and 10. minutes In the Table of the declination of the Sunne the third yeare after the Leape yeare hee found the same day after his accoumpt the obliquation of the sun in 17. 20. minuts southward which being deducted from the distance of the sunne from the Zenith because it is Southward there remaine 52. degrees and 50. minuts which is the latitude or altitude of the Pole of the Citie of Enchuysen In the yeare 1588. the 8. of Iuly at London the meridian altitude of the Sunne was obserued 59. degrees 28. minuts VVherefore his distaunce from the Zenith is 30. degrees 32. minuts In the Table of the Sunnes declination for the Leape yeare I find for that day the Suns Northren Obliquation 21. degrees 2. minuts which added to the Sunnes distance from the Zenith because it is Northerly maketh the whole 51. degrees 34. minuts which is the true latitude of the place or altitude of the Pole for the Citie of London ❧ THE DECLINATION OF THE SVNNE for the first yeere after the Leape yeere Ianuarie Februarie Marche   Aprill May. Iune Iuly August Septēber   October Nouem Decemb. Da. De. Mi Da. De Mi. Da. De. Mi.   Da. De. Mi Da. De. Mi Da. De Mi. Da De Mi. Da. De. Mi Da. De. Mi. Da De. Mi. Da. De. Mi. Da. De. Mi 1 21 43 1 13 48 1 3 30   1 8 27 1 17 55 1 23 6 1 22 9 1 15 21 1 4 36 1 7 2 1 17 31 1 23 3 2 21 33 2 13 28 2 3 7   2 8 49 2 18 10 2 23 10 2 22 1 2 15 3 2 4 13 2 7 25 2 17 47 2 23 8 3 21 23 3 13 8 3 2 44   3 9 11 3 18 25 3 23 14 3 21 53 3 14 45 3 3 50 3 7 48 3 18 3 3 23 12 4 21 12 4 12 48 4 2 20   4 9 32 4 18 40 4 23 17 4 21 44 4