植物生命的起源—— 陨击能量模型与生物能量模型的统一性 陆 玲(广州市 万归一科技发展有限公司) 【摘要】“陨击是太阳系普遍而广泛的地质过程”,地球也不例外。 基于对地壳的陨击成因、以及银河系天体螺旋运动和粒子结构的认知、以及在陨击能量模型与地球各类生物形态进行比较、地表岩层的陨击构造与植物生物区系对应性等探究过程中,地球生物,包括菌类、植物、动物的形态特征呈现出与陨击能量模型(模拟)高度的相似、生物发育秩序与陨击能量模型发展过程的高度一致。本研究认为,它们提供了说明包括植物在内的地球生命起源机制的关键线索。 外天体在陨击地表的过程中,其超强的势能转化为动能、热能和原子能等高能物理过程,导致陨落天体的基本物质——粒子的裂变和聚变,当这些粒子的构造处于膨胀,能量信息相互交换的状态,便可以受到其所处的高能物理环境的影响:“记忆”陨击过程能量运动的时空秩序,从而建立起相应的能量模型。它们作为地球生命的胚种,在特定的条件下,已记忆的信息可依序“表达”,例如“基因模型”。 植物的能量模型对应着陨击能量模型主索断裂前的阶段,动物能量模型则延续到其后阶段。陨击过程形成的生命胚种在地球特定的生态环境中,持续萌发、演变。 Origin of Plant Life Unity of Meteorite Strike Energy Model andBioenergetic Model Lu Ling (Abstract) Meteorite strike is a common and extensive geologicalprocess in the solar system, the Earth is no exception. Based on the causes ofmeteorite impact on the earth's crust, the cognition to celestial spiral motionand particle structure in the galaxy, as well as the comparison betweenmeteorite strike energy model and various biomorph on the earth, matchingbetween meteorite strike structure on ground rock stratum and plant and biota,it is inferred that the morphological characteristics of the life on the Earth,including fungi, plants and animals is highly consistent with the developmentof meteorite strike energy model. This study suggests that the said factprovides the key clue proving the mechanism of the origin of life, includingplants, on the Earth. In the course of celestialbodies hitting the earth's surface, the superior potential energy convertedinto high-energy physics process such as kinetic energy, thermal energy andnuclear energy, causing the fission and fusion of the particles, the basicmaterial objects of falling celestial bodies, when the structure of theseparticles is swelling, and the energy information exchanges, the space-timeorder of energy movement during the meteorite strike process can bememorized. As the germ of life on the Earth and under certainconditions, the information they have memorized can express in sequence, suchas gene models. Plant energy model corresponds to the phase before the main clue ofmeteorite strike energy model ruptured, while the animal energy model extendedto a later phase. The life embryo created during the meteorite strike processcontinued to develop and evolve under the specific ecological environment onthe Earth.
;+ ;NAME: ; querynednh ;PURPOSE: ; Query the HI column density of the LAB Survey for given position ;CALLING SEQUENCE: ; result=querynednh(ra,dec) ;EXAMPLE: ; IDL ra=2.018361*15 ; IDL dec=0.56667 ; IDL result=querynednh(ra,dec) ; IDL print,result ; 2.1600001e+20 ; ; IDL result=querynednh(ra,dec,/two) ; IDL print,result ; 2.1600001 ; ;PROCESS: ; webget( ),Euler ;INPUT: ; ra ---- right Longitude in degrees (sclar or veltor) ; dec ---- Latitude in degrees (sclar or veltor) ;OPTIONAL KEYWORD INPUT: ; /nearest ----- if set it, will give the HI column density of the ; nearest position of the selected position. ; default it, will give the HI column density of the ; selected position. ; /two ---- if set it, will give the HI column density in ; Unit :10^20 cm^-2 ; default it, will give the HI column density in cm^-2 ;OUTPUT: ; nh ---- the HI column density of line-of-sight ;METHOD: ; see: ; http://www.astro.uni-bonn.de/%7Ewebrai/english/tools_labsurvey.php ; by integrating over the velocity range from -400 to +400 km/s in ; the LSR frame. ; ; Kalberla,P.M.W.,Burton,W.B.,Hartmann,Dap,Arnal,E.M.,Bajaja,E., ; Morras, Poppel,W.G.L.(2005),AA,440,775 ; ; Bajaja,E.,Arnal, E.M., Larrarte,J.J., Morras, R., Poppel, ; W.G.L., Kalberla, P.M.W. 2005, AA, 440, 767 ; ; Arnal, E. M., Bajaja, E., Larrarte, J. J., Morras, R., ; Poppel, W. G. L. 2000, AAS, 142, 35 ; ; Hartmann Burton 1997, Cambridge University Press, ISBN ; 0521471117 ; ;REVISIONHISTORY: ; ORiginal by DL.Wang,26-Jun-2007 ; chage the weblink as follow: ; http://www.astro.uni-bonn.de/~webaiub/english/tools_labsearch.php ; by DL.Wang,Sep-22-2008 ; add !VERSION.OS check by DL.Wang,Oct-27-2011 ;- ;++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ Function querynednh_lab, ra, dec, nearest=nearest, two=two if N_params() lt 2 then begin print,'Syntax - info = querynednh(ra, dec)' print,' RA (degrees), Dec (degrees) -- search coordinates' endif if !VERSION.OS_family eq 'Windows' then stop euler,ra,dec,glon,glat,select=1 glon0=string(glon) glat0=string(glat) QueryURL = 'http://www.astro.uni-bonn.de/~webaiub/english/tools_labsearch.php?alpha='+strtrim(glon0,2)+'beta='+strtrim(glat0,2) result=webget(QueryURL) na=n_elements(result.text) ear=strarr(na) for i=0L,na-1 do begin ear =result.text print,i,' ',ear endfor t=result.text if not keyword_set(nearest) then begin t =strtrim(t ,1) nh0=strmid(t ,18,5) nh1=strmid(t ,38,2) nh=float(nh0)*10.0D0^float(nh1) endif else begin t =strtrim(t ,1) nh0=strmid(t ,18,5) nh1=strmid(t ,38,2) nh=float(nh0)*10.0D0^float(nh1) endelse if not keyword_set(two) then begin nh=nh endif else begin nh=nh*1.0D-20 endelse return,nh End ;++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ Function querynednh,ra, dec, nearest=nearest, two=two n=n_elements(ra) nh=dblarr(n) if not keyword_set(nearest) and not keyword_set(two) then begin for i=0L,n-1 do begin nh =querynednh_lab(ra ,dec ) endfor endif if not keyword_set(nearest) and keyword_set(two) then begin for i=0L,n-1 do begin nh =querynednh_lab(ra ,dec ,/two) endfor endif if keyword_set(nearest) and not keyword_set(two) then begin for i=0L,n-1 do begin nh =querynednh_lab(ra ,dec ,/nearest) endfor endif if keyword_set(nearest) and keyword_set(two) then begin for i=0L,n-1 do begin nh =querynednh_lab(ra ,dec ,/nearest,/two) endfor endif return,nh End
Pro ciao_prop_colden,ra,dec,nh_gal,ciao_path=ciao_path, $ upload_file=upload_file,output_file=output_file ;+ ;NAME: ; ciao_prop_colden ;PURPOSE: ; Calculate the Total Galactic H I Column Density by CIAO ; prop_colden ;INUT: ; RA: Right ascension in decimal degrees, numeric scalar or vector ; DEC: Declination in decimal degrees, numeric scalar or vector ;OPTIONAL KEYWORD INPUT: ; ciao_path: path to 'ciao.csh', default it is ; '/data/software/chandra/ciao-4.0/bin/' ; upload_file: name for uploading by CIAO prop_colden ; default it is 'ciao_prop_colden_upload' ; output_file: name for outputing by CIAO prop_colden ; default it is 'ciao_prop_colden_upload.out' ;METHOD: ; see http://chandra.ledas.ac.uk/ciao/ahelp/colden.html ;REVISION HISTORY: ; Original by DL.Wang,Sep-22-2008 ;- ;============================================================ ; STEP 1: build the data file for inputing CIAO prop_colden ;============================================================ ;Precess positions from J2000.0 (FK5) to B1950.0 (FK4) bprecess, ra, dec, ra_1950, dec_1950 ;Return RA and Dec as character string(s) in sexigesimal format radec=adstring(ra_1950, dec_1950, 1) ;Print data into file if n_elements(upload_file) eq 0 then upload_file='ciao_prop_colden_upload' openw,lun,upload_file,/get_lun for i=0L,n_elements(ra)-1 do printf,lun,radec ,format='(A27)' free_lun,lun ;============================================================ ; STEP 2: Calculate the Total Galactic H I Column Density ; by CIAO prop_colden ;============================================================ if n_elements(output_file) eq 0 then output_file='ciao_prop_colden_upload.out' if n_elements(ciao_path) eq 0 then ciao_path='/data/software/chandra/ciao-4.0/bin/' spawn,'source '+ciao_path+'ciao.csh' spawn,'prop_colden'+' :'+upload_file+':'+output_file ;============================================================= ; STEP 3: get the Total Galactic H I Column Density ; from output file ;============================================================= readcol,output_file,format='X,X,X,X,X,X,X,X,F',skipline=4,nh_gal print,'NH (10**20 per cm**2)' End